Qu Qinyue
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Qu Qinyue () (born 21 May 1935) is a Chinese astrophysicist and writer. He is a professor and former president of
Nanjing University Nanjing University (NJU; ) is a national public research university in Nanjing, Jiangsu. It is a member of C9 League and a Class A Double First Class University designated by the Chinese central government. NJU has two main campuses: the Xian ...
. He is a pioneer of high-energy astrophysics in China, and his research mainly focuses on
pulsars A pulsar (from ''pulsating radio source'') is a highly magnetized rotating neutron star that emits beams of electromagnetic radiation out of its magnetic poles. This radiation can be observed only when a beam of emission is pointing toward E ...
,
neutron stars A neutron star is the collapsed core of a massive supergiant star, which had a total mass of between 10 and 25 solar masses, possibly more if the star was especially metal-rich. Except for black holes and some hypothetical objects (e.g. white ...
, X-ray sources, γ-ray sources and
quasars A quasar is an extremely luminous active galactic nucleus (AGN). It is pronounced , and sometimes known as a quasi-stellar object, abbreviated QSO. This emission from a galaxy nucleus is powered by a supermassive black hole with a mass rangi ...
. In 1980 he was elected a member of the
Chinese Academy of Sciences The Chinese Academy of Sciences (CAS); ), known by Academia Sinica in English until the 1980s, is the national academy of the People's Republic of China for natural sciences. It has historical origins in the Academia Sinica during the Republi ...
.


Life and career

Qu Qinyue was born in Mouping, Shandong. His father was a merchant and his mother a housewife. He received his early education at Yantai Jinglun Street Primary School. Later he attended Yantai No. 1 Middle School, Zhifu Middle School and Qingdao Jiao'ao Middle School, finally graduating from Lixian Middle School. He then finished his senior high school study at Qingdao No. 1 High School.《科学家传记大辞典》编辑组 (ed.)(1994). 中国现代科学家传记 第5集. 北京市:科学出版社. . In 1953 he entered
Nanjing University Nanjing University (NJU; ) is a national public research university in Nanjing, Jiangsu. It is a member of C9 League and a Class A Double First Class University designated by the Chinese central government. NJU has two main campuses: the Xian ...
, where he studied astronomy, mathematics and physics. His teachers included astronomer Dai Wensai. In his sophomore year he proposed a wall newspaper named ''Academic Garden'', where he and his classmates posted their ideas for learning. He was also a good athlete, in 1956 his team broke the school record in the 4 × 100 m relay. After graduating in 1957, Qu became a teaching assistant of Nanjing University. In 1958 he took part in the development of China's first solar tower, and corrected an error in the design of image rotation mirror by a Soviet scholar. During the
Cultural Revolution The Cultural Revolution, formally known as the Great Proletarian Cultural Revolution, was a sociopolitical movement in the People's Republic of China (PRC) launched by Mao Zedong in 1966, and lasting until his death in 1976. Its stated goa ...
, he was sent to work at a coal mine, and then at Liyang Farm. He was unable to return to the university until 1971. After 1973, astrophysics research at Nanjing University was revived. Some of Qu's most important work was done in the late 1970s. Qu became a full professor in 1978, and a member of the
Chinese Academy of Sciences The Chinese Academy of Sciences (CAS); ), known by Academia Sinica in English until the 1980s, is the national academy of the People's Republic of China for natural sciences. It has historical origins in the Academia Sinica during the Republi ...
in 1980. In 1982 he became a member of Ministry of Education Science Textbook Compilation Committee and director of its Department of Astronomy. From 1984 to 1997, he served as President of
Nanjing University Nanjing University (NJU; ) is a national public research university in Nanjing, Jiangsu. It is a member of C9 League and a Class A Double First Class University designated by the Chinese central government. NJU has two main campuses: the Xian ...
. In August 1990 he and five other university presidents (including Lu Yongxiang) cosigned a letter to the premier
Li Peng Li Peng (; 20 October 1928 – 22 July 2019) was a Chinese politician who served as the fourth Premier of the People's Republic of China from 1987 to 1998, and as the Chairman of the Standing Committee of the National People's Congress, Ch ...
, requesting more support on universities during the 8th five-year plan. The academic ranking of Nanjing University rose rapidly under his leadership. In 1992 he was elected President of the
Chinese Astronomical Society Chinese can refer to: * Something related to China * Chinese people, people of Chinese nationality, citizenship, and/or ethnicity **''Zhonghua minzu'', the supra-ethnic concept of the Chinese nation ** List of ethnic groups in China, people of va ...
, and in 1993 a member of
TWAS The World Academy of Sciences (TWAS) is a merit-based science academy established for developing countries, uniting 1,000 scientists in some 70 countries. Its principal aim is to promote scientific capacity and excellence for sustainable deve ...
.


Work

In 1976, Qu and his colleagues developed statistical curves on pulsar energy loss rates, and suggested that JP 1953 is a pulsar. On 5 March 1979, an intense burst of hard X-rays and γ-rays was recorded, and Qu's team analyzed its
light curve In astronomy, a light curve is a graph of light intensity of a celestial object or region as a function of time, typically with the magnitude of light received on the y axis and with time on the x axis. The light is usually in a particular frequ ...
and
energy spectrum A spectrum (plural ''spectra'' or ''spectrums'') is a condition that is not limited to a specific set of values but can vary, without gaps, across a continuum. The word was first used scientifically in optics to describe the rainbow of colors ...
. They created a model for a
neutron star A neutron star is the collapsed core of a massive supergiant star, which had a total mass of between 10 and 25 solar masses, possibly more if the star was especially metal-rich. Except for black holes and some hypothetical objects (e.g. w ...
binary system A binary system is a system of two astronomical bodies which are close enough that their gravitational attraction causes them to orbit each other around a barycenter ''(also see animated examples)''. More restrictive definitions require that th ...
, and provided detailed explanation of the observational data using the mechanism of
Bremsstrahlung ''Bremsstrahlung'' (), from "to brake" and "radiation"; i.e., "braking radiation" or "deceleration radiation", is electromagnetic radiation produced by the deceleration of a charged particle when deflected by another charged particle, typicall ...
and Kruskal-Schwarzschild instability. Their work was reported at the 17th International Cosmic Ray Conference held in 1981. About the same time, Fang Lizhi, Qu Qinyue, Wang Zhenru and others proposed a theory that abnormal neutron stars, in which neutrons are in a state that their effective mass become zero or nearly zero, are a form of stars during their final period. They studied the stability of these stars, and suggested their maximum mass is approximately 4
solar masses The solar mass () is a standard unit of mass in astronomy, equal to approximately . It is often used to indicate the masses of other stars, as well as stellar clusters, nebulae, galaxies and black holes. It is approximately equal to the mass of ...
, about twice the
Tolman–Oppenheimer–Volkoff limit The Tolman–Oppenheimer–Volkoff limit (or TOV limit) is an upper bound to the mass of cold, nonrotating neutron stars, analogous to the Chandrasekhar limit for white dwarf stars. If the mass of the said star reaches the limit it will collapse to ...
. Their results demonstrated that meta-stable compact stars can exist. During the 1990s, Qu's team created new models to explain the relation between X-ray luminosity of plerionic supernova remnants and rotational energy loss rates of their central supernova. They interpreted the special shapes of some supernova remnants, such as CTB109. SS 433 was another subject they studied, calculating physical characteristics and parameters of its infrared knots. His team also discussed a fourteenth century supernova's relationship with the γ-ray source 2CG353+16. In 1993, Qu co-authored a textbook titled ''Stellar Atmosphere Physics'' (《恒星大气物理》) with Wang Zhenru.Lu Jiaxi (ed.) (1994). 中国当代科技精华 物理学卷. 哈尔滨市:黑龙江教育出版社. pp. 202–203.


References

{{DEFAULTSORT:Qu, Qinyue 1935 births Living people Chinese astrophysicists Educators from Shandong Members of the Chinese Academy of Sciences Nanjing University alumni Academic staff of Nanjing University People's Republic of China science writers Physicists from Shandong Presidents of Nanjing University Writers from Yantai