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Extractions: Antony Hewish (born Fowey Cornwall May 11 ) is a British radio astronomer who won the Nobel Prize for Physics in for his role in the discovery of pulsars. He entered the field of radio astronomy, working at the Cavendish Laboratory Cambridge , after war service in military radar research. Hewish made both practical and theoretical advances in the observation and exploitation of the apparent scintillations of radio sources due to their radiation impinging upon plasma This led him to propose, and secure funding for, the construction of a large array radio telescope at Cambridge in order to conduct a high resolution radio sky survey. In the course of this project, one of his graduate students, Jocelyn Bell, first noticed the radio source which was ultimately recognised as the first pulsar. The paper announcing the discovery had five authors, Hewish's name being listed first, Bell's second. The Nobel award to Hewish without the inclusion of Bell as a co-recipient was controversial, and was roundly condemned by Hewish's fellow astronomer Fred Hoyle Antony Hewish This content from wikipedia is licensed under the GNU Free Documentation License Power Supplies Hardware Information Law Advice
Extractions: Encyclopedia worldwide This article could be outdated : Visit our new Table of Contents Main Page Edit this page Antony Hewish (born Fowey, Cornwall, May 11 ) is a British radio astronomer who won the Nobel Prize for Physics in for his role in the discovery of pulsars. He entered the field of radio astronomy, working at the Cavendish Laboratory Cambridge , after war service in military radar research. Hewish made both practical and theoretical advances in the observation and exploitation of the apparent scintillations of radio sources due to their radiation impinging upon plasma This led him to propose, and secure funding for, the construction of a large array radio telescope at Cambridge in order to conduct a high resolution radio sky survey. In the course of this project, one of his graduate students, Jocelyn Bell, first noticed the radio source which was ultimately recognised as the first pulsar. The paper announcing the discovery had five authors, Hewish's name being listed first, Bell's second. The Nobel award to Hewish without the inclusion of Bell as a co-recipient was controversial, and was roundly condemned by Hewish's fellow astronomer
Anecdote - Antony Hewish - LGM-1 the Nobel Prize). hewish, antony (1924 ) British astronomer, Nobel Prize recipient(Physics, 1974) noted for his discovery of pulsars Sources Karnataka http://www.anecdotage.com/index.php?aid=5964
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Extractions: see previous page Antony Hewish (born Fowey Cornwall May 11 ) is a British radio astronomer who won the Nobel Prize for Physics in for his role in the discovery of pulsars. He entered the field of radio astronomy, working at the Cavendish Laboratory Cambridge , after war service in military radar research. Hewish made both practical and theoretical advances in the observation and exploitation of the apparent scintillations of radio sources due to their radiation impinging upon plasma This led him to propose, and secure funding for, the construction of a large array radio telescope at Cambridge in order to conduct a high resolution radio sky survey. In the course of this project, one of his graduate students, Jocelyn Bell, first noticed the radio source which was ultimately recognised as the first pulsar. The paper announcing the discovery had five authors, Hewish's name being listed first, Bell's second. The Nobel award to Hewish without the inclusion of Bell as a co-recipient was controversial, and was roundly condemned by Hewish's fellow astronomer
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Skolavpohode.cz hewish, antony (1924) antony hewish vystudoval na universite v Cambridi av roce1946 se stal clenem radioastronomické skupiny pod vedením Martina Ryla . http://www.skolavpohode.cz/clanek.asp?polozkaID=3653
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Hewish - En De Ontdekking Van Pulsar. Wie was hewish? antony hewish is geboren op 11 mei 1924 in Fowey, Cornwall inEngeland. (home). antony hewish en Martin Ryle. Hoe gaat het nu met hewish? http://anw.hml.nl/Werkstukken/Lotte_Caarls/hewish/
Extractions: E mei 2002 Wie was Hewish? Wat is pulsar? Hoe is pulsar ontdekt? Hoe is het onderzoek naar pulsars verder verlopen? ... Bronvermelding. Antony Hewish is geboren op 11 mei 1924 in Fowey, Cornwall in Engeland. Op zijn achttiende ging Hewish studeren aan de universiteit van Cambridge. Hier stopte hij tijdelijk mee in 1943 doordat hij opgeroepen was om aan het front te gaan strijden, hier werkte hij onder andere met radarmeetapparatuur. In 1946 keerde hij terug naar de universiteit en studeerde daar in 1948 af. In 1952 besloot Hewish zich te specialiseren in radioastronomie. In dit gebied heeft hij enkele ontdekkingen gedaan, waarvan de grootste en belangrijkste de ontdekking van pulsar was. Later is hij les gaan geven. Hij is professor in de radioastronomie geworden, en in 1977 werd hij hoofd van de radioastronomiesectie van de universiteit van Cambridge. In 1950 is Hewish getrouwd, hij heeft 2 kinderen gekregen. Hewish en zijn vrouw Prijzen die Antony Hewish mocht ontvangen zijn onder andere: Hamilton Prize, Cambridge (1952); Eddington Medal, Royal Astronomical Society (1969); Charles Vernon Boys Prize, Institute of Physics (1970); Dellinger Medal, International Union of Radio Science (1972); Michelson Medal, Franklin Institute (1973); Hopkins Prize, Cambridge Philosophical Society (1973); Holwech Medal and Prize, Societé Française de Physique (1974); Nobel Prijs in Natuurkunde (1974); Hughes Medal, Royal Society (1976), en hij heeft nog veel meer prijzen gekregen.
Nobel Laureate In 1974 antony hewish. (1924 ?) In 1974 antony hewish received the NobelPrice for his great work in physics. British astrophysicist who http://www.freewebs.com/nobelprize/A_Hewish.htm
Extractions: Hewish was educated at the University of Cambridge and in 1946 joined the radio astronomy group there led by Sir Martin Ryle. While directing a research project at the Mullard Radioastronomy Observatory at Cambridge 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. For this work in identifying pulsars as a new class of stars, he was awarded jointly with Ryle the Nobel Prize for Physics in 1974, the first time the prize had been given for observational astronomy.
Jocelyn Bell Private communication, March 10, 1997, . hewish, antony. hewish, antony, et al(1968) Nature, 217, 709713, Observation of a Pulsating Radio Source . http://aci.mta.ca/courses/physics/1001/Misc/StudentPapers97/Bell.html
Extractions: Gender equality in science is a frequently discussed issue in today's society. An enormous amount of progress is being made by women in areas in which they were previously under-represented. One such example is the work of Jocelyn Bell in the field of astrophysics. As a graduate student at Cambridge University in 1967, Bell discovered evidence of a new type of star in our galaxy called pulsars. Prior to this, pulsars, or pulsating neutron stars, had only been a theory, and this evidence established a foundation from which to expand and verify the theory. Due to scientific hierarchies and reward systems, however, the work and discovery was accredited to Bell's professor, Antony Hewish, thus creating a veritable astronomical injustice in the form of the Jocelyn Bell story. Pulsars served to prove this theory of star rotation. Perhaps the greatest verification comes from the Crab Nebula. Documented by Chinese astronomers in 1054, a supernova explosion created the luminous remains known as the Crab Nebula.(Stellar Evol., p.54) The source for the luminosity was unknown until the presence of a high density pulsar was discovered near its centre. The rate of rotation of this galactic object is about 33 ms, which is much quicker than the average pulsar period of 1.34 seconds.(Hewish, p.740) To be rotating at such a fast speed, the star had to be extremely compact. However, with such pulse precision and energy output, the star also had to be extremely massive. A high density star would allow for both characteristics, and the detection of the Crab Nebula pulsar thus helped to substantiate the claims for a rotating star.
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