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  1. Antony Hewish
  2. Pulsars and High Density Physics. by Antony. HEWISH, 1975
  3. Pulsars and High Density Physics. pp. 70-79 IN: Les Prix Nobel en 1974 by Antony. HEWISH, 1975

61. Making Contact With Pulsars
In 1974, they awarded the Nobel Prize in Physics to antony hewish and Sir MartinRyle (leader of the Cambridge radio astronomy group).
http://hypatiamaze.org/j_bell/pulsar.html
The real story behind the discovery of pulsars by astronomer Jocelyn Bell
MAKING
with JOCELYN BELL BURNELL
There is no doubt that Carl Sagan borrowed a lot from science history in writing his novel Contact. Science history! you say. Have we been contacted by aliens and traveling through worm holes? No, but the first part of the story is so similar to the real life story of Jocelyn Bell who discovered pulsars in 1967, some of the opening scenes from the movie could have been taken from the TV documentary about Bell.
Interactive Timeline of Space Discovery
True, the movie Contact features the giant dish antennae radio telescopes and not the type (a field of wires) built by Jocelyn and fellow students from a design by Antony Hewish, her advisor. And the location was switched from Cambridge, England to the deserts of Socorro , New Mexico.
Nevertheless, there is Jody Foster on screen analyzing what Jocelyn called "bits of scruff" - very faint signals which appeared on her print out frequently, and more important, in regular cycles (every 1.337 seconds with a duration of 0.3 sec.)
What was the source of these signals? Was it an orbiting satellite? Radar? Or possibly French TV signals bouncing across the English Channel? The signals occurred 4 minutes earlier each evening just like the stars rising in the sky. With the earthly possibilites ruled out, Hewish even considered "little green men" from outer space who were trying to reach us by radio. The press went wild.

62. Research In Review At Florida State University
graduate student working for astronomer antony hewish in Cambridge, England.She and hewish had just finished building a new radio telescope,
http://www.research.fsu.edu/researchr/summer2005/features/starstuff.html
Features > Star Stuff Summer 2005 Cover Story Features Departments Cover ... FSU Home Star Stuff By Don Wood Little green men. The unwelcome thought wouldn’t go away. But how else could she explain those tiny squiggles coming from her chart recorder? Bell, in charge of the telescope, was making observations toward her Ph.D. Bell decided she needed more detail on the odd blips, so she installed a faster chart recorder (this was before the age of ubiquitous computers) to get a clearer picture. For two months nothing showed up. Then the mysterious signal reappeared. The new recorder showed that the radio pulses were coming at an unvarying interval of 1.33 seconds. Exactly every one point three three seconds, with not a fraction of variance. Logic dictated that if the signals were indeed artificial, they must be coming from intelligent aliens. Little green men. Bell dubbed the source LGM-1 (the first “little green men” signal) and continued her observations while she, Hewish and the others debated how to announce their discovery. They didn’t really believe the signals were coming from aliens, but they were at a loss for any natural explanation. And then Bell found another source, and soon another, and another, all in different parts of the sky and all showing the same regularity (but with slightly different periods). It seemed very unlikely that four groups of aliens were all broadcasting at the same frequency. Bell and Hewish quickly dropped the LGM hypothesis.

63. ScienceWeek
and although her supervisor antony hewish later received a Nobel Prize at Cambridge University, under the direction of my adviser, antony hewish.
http://scienceweek.com/2004/sc040611-1.htm
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ScienceWeek 2004 11 June C1 PULSARS AND WOMEN IN ASTRONOMY
Jocelyn Bell, now known as S. Jocelyn Bell Burnell, was the de facto discoverer of the first pulsar in 1967. She was a graduate student at that time, and although her supervisor Antony Hewish later received a Nobel Prize for the discovery, Jocelyn Bell was not included.
The following points are made by S. Jocelyn Bell Burnell (Science 2004 304:489):
1) Pulsars are phenomenal objects: rapidly rotating neutron stars that send out beams of radio waves which, like lighthouse beams, sweep around the sky as the star rotates. They are amazingly precise timing devices that can be used as clocks for testing relativity theory and may be used for timekeeping and navigation. With a diameter of only about 15 kilometers and a density comparable to that of the nucleus of an atom, they also provide a laboratory for some extreme physics.
2) In the fall of 1967, I was conducting a routine mapping project studying the radio scintillation of quasars for my doctoral thesis at Cambridge University, under the direction of my adviser, Antony Hewish. Investigation of a puzzling weak signal showed it to be a string of pulses, 1.33 seconds apart. We spent a month trying to find out what was wrong, so unexpected was the signal; and we nicknamed it "Little Green Men" (LGM). At the end of that month, I found a second pulsar, killing the LGM hypothesis and indicating a new kind of astronomical source.

64. Cambridge Minds - Cambridge University Press
Radioastronomy in Cambridge antony hewish; 5. Ray Monk, Stephen Heath, GillianSutherland, antony hewish, Colin Renfrew, Geoffrey Harcourt, Jeremy Gray,
http://www.cambridge.org/uk/catalogue/catalogue.asp?isbn=0521456258

65. August/September 2005 Supplemental Info
The telescope was designed by Cambridge radio astronomer antony hewish to searchfor quasars, and it was Bell s job to analyze its river of data.
http://www.airandspacemagazine.com/ASM/Mag/Supp/AS05/EUFS.html
Einstein's Unfinished Symphony
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CONTENTS
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Martin/Convair
Skywalking in a T-38

Einstein's Unfinished
P-47 Walkaround

Flying Despots

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Prop Art
... Home Page LINKS We had a hundred feet of chart paper every day, seven days a week, and I operated it for six months, which meant I was personally responsible for quite a few miles of chart recording. It was four hundred feet of chart paper before you got back to the same bit of sky, and I thought-having had all these marvelous lectures as a kid about the scientific method-that this was the ideal way to do science. With that quantity of data, no way are you going to remember what happened four hundred feet ago. You're going to come to each patch of sky absolutely fresh, and record it in a totally unbiased way. But actually, one underestimates the human brain. On a quarter inch of those four hundred feet, there was a little bit of what I call "scruff," which didn't look exactly like [quasar] scintillation....After a while I began to remember that I had seen some of this unclassifiable scruff before, and what's more, I had seen it from the same patch of sky. The 81.5-megahertz radio signal was emanating from a spot midway between the stars Vega and Altair. A higher-speed recording revealed that the signal was actually a precise succession of pulses spaced 1.3 seconds apart. The unprecedented clocklike beeps caused Hewish and his group to label the source LGM for "Little Green Men." This was done only half in jest. At one point some consideration was given to the possibility that the regular pulsations were coming from a beacon set up by an extraterrestrial civilization. Within a month Bell ferreted out, from the yards upon yards of strip chart that were spewing from the telescope, the telltale markings of a second suspicious source. Its period was 1.19 seconds. By the beginning of 1968, two more were uncovered. When the phenomenon was announced to the public, a British journalist dubbed the freakish sources pulsars.

66. Royal Society | About The Society | About Us | The Fellowship | Directory Of Fel
hewish, Professor antony FRS. Elected , 1968. Medal(s) , Hughes (1977).Nobel Prizes , Physics (1974). Email a friend Printer friendly. Select area
http://www.royalsoc.ac.uk/view_fellow.cfm?FID=660

67. StarChild: Did You Know... (Jocelyn Bell Burnell)
the Nobel Prize in physics was jointly awarded to astronomers antony hewishand Sir Martin Ryle. antony hewish was honored for the discovery of pulsars.
http://starchild.gsfc.nasa.gov/docs/StarChild/whos_who_level2/bell_know.html
Did you know...?
In 1974, the Nobel Prize in physics was jointly awarded to astronomers Antony Hewish and Sir Martin Ryle. Antony Hewish was honored for the discovery of pulsars. Many have argued that Jocelyn Bell Burnell should have shared that honor. Show me a printable version of this page.
Return to the StarChild Main Page

Go to Imagine the Universe!
(A site for ages 14 and up.)
The StarChild site is a service of the High Energy Astrophysics Science Archive Research Center (HEASARC) Dr. Nicholas E. White (Director) , within the Exploration of the Universe Division (EUD) at NASA/ GSFC StarChild Authors: The StarChild Team
Acknowledgments

StarChild Project Leader: Dr. Laura A. Whitlock
Responsible NASA Official: Phil Newman
If you have comments or questions about the StarChild site, please send them to starchild@heasarc.gsfc.nasa.gov NASA's Privacy Statement NASA's Security Statement

68. Jocelyn Bell Burnell
It was while she was a graduate student at Cambridge, working under the directionof antony hewish, that Jocelyn Bell discovered pulsars.
http://starchild.gsfc.nasa.gov/docs/StarChild/whos_who_level2/bell.html
Jocelyn Bell Burnell
Can You Believe It? When they were not sure what caused the signals they detected, Jocelyn Bell and her college advisor D. Anthony Hewish labeled the signal LGM for Little Green Men. They thought it could possibly be a beacon from an alien source. Susan Jocelyn Bell was born in Belfast, Northern Ireland on July 15, 1943. Her father was an architect and an avid reader. Through his books, Jocelyn was introduced to the world of astronomy. Her family and the staff of the Armagh Observatory, which was near her home in Belfast, encouraged her interest in astronomy. Jocelyn Bell's parents very strongly believed in educating women. When she failed the examination required for students wanting to pursue higher education in British schools, they sent her to a boarding school to continue her education. In 1965, Jocelyn Bell earned a B.S. degree in physics from the University of Glasgow. Later that same year she began work on her Ph.D. at Cambridge University. It was while she was a graduate student at Cambridge, working under the direction of Antony Hewish, that Jocelyn Bell discovered pulsars.

69. Nobel Prizes In Physics
antony hewish. British. astrophysics. 1975. Aage Bohr. Danish. atomic structure.1975. Ben Mottelson hewish, antony. Martin Ryle. 1952. Cambridge
http://www.chem.yorku.ca/NAMED/NOBEL/PHYS/
Nobel Prizes in Physics
Department of Chemistry, York University
4700 Keele Street, Toronto, ONTARIO M3J 1P3, CANADA For suggestions, corrections, additional information, and comments please send e-mails to jandraos@yorku.ca http://www.chem.yorku.ca/NAMED/ NOBEL PRIZE PHYSICS YEAR NAME OF SCIENTISTS NATIONALITY TYPE OF PHYSICS Wilhelm Conrad Roentgen German radiation Henrik Antoon Lorentz Dutch magnetism, radiation Pieter Zeeman Dutch magnetism, radiation Pierre Curie French radiation Marie Curie French radiation Antoine Henri Becquerel French radiation Lord John William Strutt Rayleigh British gases Philipp Eduard Anton Lenard Hungarian-German cathode rays Sir Joseph John Thomson British gases Albert Abraham Michelson German-American spectroscopy Gabriel Lippmann French optics Guglielmo Marconi Italian telegraphy Carl Ferdinand Braun German telegraphy Johannes Diderik van der Waals Dutch gases Wilhelm Wien German radiation Nils Gustaf Dalen Swedish gases Heike Kamerlingh-Onnes Dutch cryogenics Max von Laue German crystallography Sir William Henry Bragg British crystallography Sir William Lawrence Bragg British crystallography no prize awarded Charles Glover Barkla British radiation Max Planck German quantum theory, radiation

70. MSN Encarta - Hewish, Antony
Translate this page hewish, antony (Fowels 1924), astrofisico britannico a cui si deve la scopertadelle pulsar. Altre risorse di Encarta. Cerca in Encarta hewish, antony
http://it.encarta.msn.com/encyclopedia_981535973/Hewish_Antony.html

71. RASC Library - Subject Index - Alphabet E
Radio waves, hewish, antony (ed.) Seeing Beyond the Visible, 535.01 HEW, LondonEnglish Universities Press, 1970, 0, 150p. illus
http://www.rasc.ca/library/libse.htm
The Royal Astronomical Society of Canada Library
Subject Index - Alphabet E
Home Library A B ... Z Subject heading Author Title Out Dewey Note Publisher Lyear L.C. Notes Earth Chamberlin, Thomas Chrowder The Origin of the Earth 550.1 C Chicago: The University of Chicago Press Earth Hodgson, John N. 551.22 H Englewood Cliffs, N.J.: Prentice-Hall Earth Jeffreys, Harold The Earth 551 J Cambridge: University Press Earth Scientific American The Planet Earth 551 S New York: Simon and Schuster Earth
Moon
Planets Whipple, Fred L. Earth, Moon, and Planets 523.2 W Copy 1 Philadelphia: The Blakiston Company Subject heading Author Title Out Dewey Note Publisher Lyear L.C. Notes Earth
Stars Abbot, Charles G. The Earth and the Stars 523 A Copy 1 New York: Van Nostrand Earthquakes Knott, Cargill Gilston The Physics of Earthquake Phenomena 551.2 K Oxford: Clarendon Eclipses Buchanan, Roberdeau The Mathematical Theory of Eclipses 521.8 B Philadelphia, London: J.B. Lippincott Co Eclipses Chambers, George F. The Story of Eclipses 523 C London: Newnes Eclipses Lewis, Isabel Martin A Handbook of Solar Eclipses 523.78 L

72. Enciclopedia :: 100cia.com
Translate this page antony hewish. (En este momento no hay texto en esta p�gina. Para iniciar elart�culo, click editar esta p�gina (http//es.wikipedia.
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¿Sabías que Allen, Woody dijo...?
En realidad, prefiero la ciencia a la religión. Si me dan a escoger entre Dios y el aire acondicionado, me quedo con el aire.
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73. News | U-M WISE
who discovered the first radio pulsars with her thesis advisor antony hewish . At Cambridge, she worked with hewish and others to construct a radio
http://www.wise.umich.edu/news/
  • News and Events
    News and Events
    WISE sponsors talk, luncheon with Jocelyn Bell Burnell, the women who discovered pulsars
    The Women in Science and Engineering (WISE) Program is sponsoring the following events during Jocelyn Bell Burnell's (bio below) visit to the University of Michigan campus in September.
    • Graduate Women Luncheon
      Tuesday, September 20, 2006, Noon-1:30pm, Rackham's East Conference Room (4th Floor)
      Dr. Bell Burnell will speak at a luncheon aimed at female graduate women in the sciences, engineering, mathematics and statistics. Registration is required and is limited to 40. This is a free event. To register, please contact Ruth Lum at lumb@umich.edu. Physics Lecture: What Astonomy Has Done For Einstein
      Wednesday, September 21, 2006, 4:15pm, 1324 East Hall.
      This lecture is aimed at the general campus and non-campus community. No registration is required. Co-Sponsors include: WISE, Physics Dept., and Astronomy Dept. SWiP (Society of Women in Physics) Luncheon for Undergraduate Women
      Wednesday, September 21, 2006, Noon-1:30, 337 W. Hall

74. Women Of Achievement
The discovery enabled her supervisor antony hewish to win the Nobel Prize inphysics in 1974. She received no credit from the Nobel committee although the
http://www.undelete.org/woa/woa07-15.html
PRIOR DATE HOME WOA INDEX NEXT DATE July 15
Compiled and Written by Irene Stuber
who is solely responsible for its content.
07-15 TABLE of CONTENTS: Her supervisor got the Nobel for her work DATES, ANNIVERSARIES, and EVENTS QUOTE by Denise Scott Brown. Jocelyn Bell Burnell Jocelyn Bell Burnell's amazing discovery was confiscated by her supervisor who then won the Pulitzer Prize for it. That's a bit simplistically put, but does describe essentially what happened.
Born 07-15-1943, Jocelyn Bell Burnell, British astronomer and educator discovered pulsating radio stars or pulsars at age 24. The discovery enabled her supervisor Antony Hewish to win the Nobel Prize in physics in 1974.
She received no credit from the Nobel committee although the year before the Franklin Institute of Philadelphia had awarded the prestigious Michelson Medal to both Hewish and Bell.
At the time and in subsequent interviews, Bell (who wanted to continue on the field) said that it would have been unseemly for a 24-year-old to receive such honors.
Hewish made his theory announcement in 1968 after his recommendation that JBB BURY her pulsar discovery information in the appendix of her doctoral dissertation
Bell has proved her discovery at 24 was no fluke by becoming only one of two women in Great Britain to hold the position of full professor of physics. She has received a number of the most prestigious awards in astronomy.

75. TCSS Trinity College Science Society - Prof Antony Hewish FRS
Prof antony hewish FRS. Pulsar Physics. Wednesday 16.2.05; Old Combination Room,8 pm. Pulsars are stars as massive as the Sun with interior densities
http://www.trin.cam.ac.uk/tcss/hewish160205.html
Home Overview Events Archives ... Committee Prof Antony Hewish FRS Pulsar Physics Wednesday 16.2.05; Old Combination Room , 8 p.m. Pulsars are stars as massive as the Sun with interior densities exceeding 100 million tonnes per cubic cm and typical magnetic fields of 100 million Teslas. Spinning at up to 600 revs per sec they emit coherent, beamed radiation. Understanding how they behave, and how they can be used to test general relativity involves some interesting physics. Background Resources Professor Hewish is a radio astronomer who was awarded, with Martin Ryle, the Nobel Prize for Physics 1974 for his work on pulsars (rapidly rotating neutron stars that emit pulses of energy). The discovery by Jocelyn Bell Burnell of a regularly fluctuating signal, which turned out to be the first pulsar, began a period of intensive research. Professor Hewish discovered another three straight away, and more than 170 pulsars have been found since 1967. He was born in Cornwall and was educated at Cambridge. In 1946, he joined the radio astronomy group led by Sir Martin Ryle. While directing a research project at the Mullard Radioastronomy Observatory in 1967, Hewish recognized the significance of an observation made by a graduate assistant, Jocelyn Bell. He determined that the regularly patterned radio signals, or pulses, that Bell had detected were not caused by earthly interference or, as some speculated, by intelligent life forms trying to communicate with distant planets but rather were energy emissions from certain stars.

76. CUSS - Cambridge University Scientific Society
Professor antony hewish, Emeritus Professor of Radio Astronomy, Cambridge University.Fellow of Churchill College. Awarded the Nobel Prize for Physics in
http://www.srcf.ucam.org/scisoc/patrons/
Home Contact us Search document.write(messages[15]); Home About us Events Constitution ... Links Patrons of CUSS
Max Perutz, 1914 - 2002 The society mourns the death of one of its Patrons, the Nobel Laureate Max Perutz. Professor Perutz had been affiliated with the society since giving a CUSS talk on the life of Lise Meitner in 1997. He was a former head of the MRC Laboratory of Molecular Biology in Cambridge and was awarded the Nobel Prize for Chemistry in 1962 for work on the structure of haemoglobin. Please read this page for a brief tribute to his life and work.
Professor Sir Michael Atiyah OM FRS President of the Royal Society (1990-95). Master of Trinity College, Cambridge (1990-1997). Director of the Isaac Newton Institute for Mathematical Sciences. Awarded the Fields Medal at the International Congress of Mathematicians, 1966. Appointed as Chancellor of the University of Leicester beginning in July of 1996.
Professor Antony Hewish FRS Emeritus Professor of Radio Astronomy, Cambridge University. Fellow of Churchill College. Awarded the Nobel Prize for Physics in 1974 for the discovery of pulsars.

77. Nat' Academies Press, Conflict In The Cosmos: Hoyle Biography (2005)
hewish, antony, 199, 287288, 289, 326-327, 328. Hey, James, 179. Hill, Alan, 191.Hitler, Adolf, 28, 47, 56, 58, 83, 87, 96, 111. HMS Achilles, 85
http://www.nap.edu/openbook/0309093139/html/389.html
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Openbook Linked Table of Contents Front Matter, pp. i-xviii 1 An End and a Beginning, pp. 1-26 2 To the Frontiers of the Universe: Training for Cosmology, pp. 27-58 3 The Star Makers, pp. 59-82 4 Hoyle s Secret War, pp. 83-112 5 The Nature of the Universe, pp. 113-148 6 Lives of the Stars, pp. 149-176 7 Clash of Titans, pp. 177-210 8 Origin of the Chemical Elements, pp. 211-238 9 Matters of Gravity, pp. 239-274 10 Mountains to Climb, pp. 275-298 11 The Watershed, pp. 299-316 12 Stones, Bones, Bugs, and Accidents, pp. 317-348 Notes, pp. 349-368 Bibliography, pp. 369-378 Acknowledgments, pp. 379-382 Index, pp. 383-402 Photos, pp. 403-410 GO TO PAGE:
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78. Nat' Academies Press, Conflict In The Cosmos: Hoyle Biography (2005)
for the development of radio interferometers, and to antony hewish, both Tommy Gold at Cornell, who backed up Hoyle, and Professor antony hewish.
http://www.nap.edu/openbook/0309093139/html/326.html
Read more than 3,000 books online FREE! More than 900 PDFs now available for sale HOME ABOUT NAP CONTACT NAP HELP ... ORDERING INFO Items in cart [0] TRY OUR SPECIAL DISCOVERY ENGINE Questions? Call 888-624-8373 Conflict in the Cosmos: Hoyle Biography (2005)
Joseph Henry Press ( JHP
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Research ...
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NEW!
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CHAPTER SELECTOR:
Openbook Linked Table of Contents Front Matter, pp. i-xviii 1 An End and a Beginning, pp. 1-26 2 To the Frontiers of the Universe: Training for Cosmology, pp. 27-58 3 The Star Makers, pp. 59-82 4 Hoyle s Secret War, pp. 83-112 5 The Nature of the Universe, pp. 113-148 6 Lives of the Stars, pp. 149-176 7 Clash of Titans, pp. 177-210 8 Origin of the Chemical Elements, pp. 211-238 9 Matters of Gravity, pp. 239-274 10 Mountains to Climb, pp. 275-298 11 The Watershed, pp. 299-316 12 Stones, Bones, Bugs, and Accidents, pp. 317-348 Notes, pp. 349-368 Bibliography, pp. 369-378 Acknowledgments, pp. 379-382 Index, pp. 383-402 Photos, pp. 403-410 GO TO PAGE:
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PAGE PRINTABLE PDF PAGE CHAPTER PAGE SEARCH THIS BOOK: The following HTML text is provided to enhance online readability. Many aspects of typography translate only awkwardly to HTML. Please use the

79. Dickinson College - Campus News Extra
As a graduate student at Cambridge, she worked under antony hewish and aided inthe discovery of pulsarsa scientific breakthrough that ranks as an
http://cfserv.dickinson.edu/cnExtra/detail.cfm?117

80. Scientific American Digital Browse
In 1967 Jocelyn Bell and antony hewish found the first pulsar. Their radiotelescope brought in signals from a source that emitted very regular pulses every
http://www.sciamdigital.com/browse.cfm?ITEMIDCHAR=22A667AF-2B35-221B-6AA8DDA677D

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