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フランク・シュー（Frank H. Shu, 徐遐生, 1943年6月2日 - ）は、アメリカ合衆国の天文学者・天体物理学者。カリフォルニア大学バークレー校とカリフォルニア大学サンディエゴ校で天文学の教授を務めている。また、中央研究院のである。
, Frank Shu (em chinês: 徐遐生; Kunming, 2 de junho de 1943) é um astrofísico estadunidense de origem chinesa.
, Frank Hsia-San Shu (Chinese: 徐遐生; Jyutping … Frank Hsia-San Shu (Chinese: 徐遐生; Jyutping: Ceoi4 Haa4 Sang1; born June 2, 1943), is a Chinese-American astrophysicist, astronomer and author. He is currently a University Professor Emeritus at the University of California, Berkeley and University of California, San Diego. He is best known for proposing the density wave theory to explain the structure of spiral galaxies, and for describing a model of star formation, where a giant dense molecular cloud collapses to form a star. molecular cloud collapses to form a star.
, Frank Shu (chinesisch 徐遐生, Pinyin Xú Xiásh … Frank Shu (chinesisch 徐遐生, Pinyin Xú Xiáshēng; * 2. Juni 1943 in Kunming) ist ein US-amerikanischer Astrophysiker chinesischer Abstammung. Shu wurde im chinesischen Kunming geboren und kam als Sechsjähriger in die Vereinigten Staaten, wo er in Chicago und West Lafayette aufwuchs. Er erhielt 1963 den Bachelor in Physik am Massachusetts Institute of Technology. Den Doktorgrad in Astronomie erwarb er 1968 an der Harvard University, danach lehrte er fünf Jahre an der SUNY Stony Brook. 1972 erhielt er ein Forschungsstipendium der Alfred P. Sloan Foundation (Sloan Research Fellowship). Shu war von 1973 bis 2002 Professor an der University of California, Berkeley, deren Astronomie-Departement er von 1984 bis 1988 leitete. Von 2002 bis 2006 war er Präsident der National Tsing Hua University in Taiwan. Seit 2006 ist er an der University of California, San Diego, seit 2009 emeritierter Professor. Von 1994 bis 1996 war Shu Präsident der American Astronomical Society (AAS). Shu arbeitete als Theoretiker über Themen wie den Ursprung von Meteoriten, Entstehung und frühe Entwicklung von Sternen, Massentransfer in engen Doppelsternen und die Struktur von Spiralgalaxien.Noch als Student entwickelte er mit Chia-Chiao Lin die als Dichtewellentheorie bekannte Theorie der Spiralarme in Galaxien. 1977 veröffentlichte er ein Modell für die Entstehung eines Sterns durch Kollaps einer sphärischen Gaswolke im Kern einer Molekülwolke.schen Gaswolke im Kern einer Molekülwolke.
, Frank H. Shu (Hanzi: 徐遐生; Pinyin: Xú Xiásh … Frank H. Shu (Hanzi: 徐遐生; Pinyin: Xú Xiáshēng; lahir pada 2 Juni 1943) adalah seorang astrofisikawan, astronom dan penulis. Saat ini ia adalah seorang profesor emeritus dalam bidang astronomi di University of California, Berkeley dan University of California, San Diego.y dan University of California, San Diego.
, Frank Hsia-San Shu (Chinois 徐遐生 ; né le 2 … Frank Hsia-San Shu (Chinois 徐遐生 ; né le 2 juin 1943), est un astrophysicien, astronome et auteur sino-américain. Il est actuellement professeur d'université émérite à l'Université de Californie à Berkeley et à l'Université de Californie à San Diego. Il est surtout connu pour avoir proposé la théorie des ondes de densité pour expliquer la structure des galaxies spirales et pour avoir décrit un modèle de formation d'étoiles, où un nuage moléculaire dense géant s'effondre pour former une étoile.e géant s'effondre pour former une étoile.
, فرانك شو (بالإنجليزية: Frank Shu) (و. 1943 – م) هو عالم فلك، وأستاذ جامعي من الولايات المتحدة الأمريكية. ولد في كونمينغ. هو عضوٌ في الأكاديمية الوطنية للعلوم، والأكاديمية الأمريكية للفنون والعلوم.
, 徐遐生（英語：Frank Hsia-San Shu，1943年6月2日－），籍貫浙江永嘉，出生于云南昆明，美籍華人天文學家，中央研究院院士。 其父親為徐賢修，父子皆曾任國立清華大學校長。
, Фрэнк Шу (кит. трад. 徐遐生, пиньинь Xú Xiáshēng, палл. Сюй Сяшэн, р. 1943) — американский астрофизик китайского происхождения.
, Frank Shu (in lingua cinese: 徐遐生; Kunming, … Frank Shu (in lingua cinese: 徐遐生; Kunming, 1943) è un astrofisico cinese. Ha insegnato presso l'Università della California, Berkeley e all'Università della California, San Diego. Shu è conosciuto per i propri lavori pionieristici in diversi campi dell'astrofisica e dell'astronomia, inclusi studi sulla nascita delle meteoriti, la nascita e lo sviluppo iniziale delle stelle e la struttura delle galassie a spirale.e e la struttura delle galassie a spirale.
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Frank Hsia-San Shu (Chinois 徐遐生 ; né le 2 … Frank Hsia-San Shu (Chinois 徐遐生 ; né le 2 juin 1943), est un astrophysicien, astronome et auteur sino-américain. Il est actuellement professeur d'université émérite à l'Université de Californie à Berkeley et à l'Université de Californie à San Diego. Il est surtout connu pour avoir proposé la théorie des ondes de densité pour expliquer la structure des galaxies spirales et pour avoir décrit un modèle de formation d'étoiles, où un nuage moléculaire dense géant s'effondre pour former une étoile.e géant s'effondre pour former une étoile.
, Frank Shu (in lingua cinese: 徐遐生; Kunming, … Frank Shu (in lingua cinese: 徐遐生; Kunming, 1943) è un astrofisico cinese. Ha insegnato presso l'Università della California, Berkeley e all'Università della California, San Diego. Shu è conosciuto per i propri lavori pionieristici in diversi campi dell'astrofisica e dell'astronomia, inclusi studi sulla nascita delle meteoriti, la nascita e lo sviluppo iniziale delle stelle e la struttura delle galassie a spirale.e e la struttura delle galassie a spirale.
, Frank Shu (chinesisch 徐遐生, Pinyin Xú Xiásh … Frank Shu (chinesisch 徐遐生, Pinyin Xú Xiáshēng; * 2. Juni 1943 in Kunming) ist ein US-amerikanischer Astrophysiker chinesischer Abstammung. Shu wurde im chinesischen Kunming geboren und kam als Sechsjähriger in die Vereinigten Staaten, wo er in Chicago und West Lafayette aufwuchs. Er erhielt 1963 den Bachelor in Physik am Massachusetts Institute of Technology. Den Doktorgrad in Astronomie erwarb er 1968 an der Harvard University, danach lehrte er fünf Jahre an der SUNY Stony Brook. 1972 erhielt er ein Forschungsstipendium der Alfred P. Sloan Foundation (Sloan Research Fellowship). Shu war von 1973 bis 2002 Professor an der University of California, Berkeley, deren Astronomie-Departement er von 1984 bis 1988 leitete. Von 2002 bis 2006 war er Präsident der National Tsing Hua University in Tait der National Tsing Hua University in Tai
, Фрэнк Шу (кит. трад. 徐遐生, пиньинь Xú Xiáshēng, палл. Сюй Сяшэн, р. 1943) — американский астрофизик китайского происхождения.
, フランク・シュー（Frank H. Shu, 徐遐生, 1943年6月2日 - ）は、アメリカ合衆国の天文学者・天体物理学者。カリフォルニア大学バークレー校とカリフォルニア大学サンディエゴ校で天文学の教授を務めている。また、中央研究院のである。
, Frank Shu (em chinês: 徐遐生; Kunming, 2 de junho de 1943) é um astrofísico estadunidense de origem chinesa.
, فرانك شو (بالإنجليزية: Frank Shu) (و. 1943 – م) هو عالم فلك، وأستاذ جامعي من الولايات المتحدة الأمريكية. ولد في كونمينغ. هو عضوٌ في الأكاديمية الوطنية للعلوم، والأكاديمية الأمريكية للفنون والعلوم.
, Frank H. Shu (Hanzi: 徐遐生; Pinyin: Xú Xiásh … Frank H. Shu (Hanzi: 徐遐生; Pinyin: Xú Xiáshēng; lahir pada 2 Juni 1943) adalah seorang astrofisikawan, astronom dan penulis. Saat ini ia adalah seorang profesor emeritus dalam bidang astronomi di University of California, Berkeley dan University of California, San Diego.y dan University of California, San Diego.
, Frank Hsia-San Shu (Chinese: 徐遐生; Jyutping … Frank Hsia-San Shu (Chinese: 徐遐生; Jyutping: Ceoi4 Haa4 Sang1; born June 2, 1943), is a Chinese-American astrophysicist, astronomer and author. He is currently a University Professor Emeritus at the University of California, Berkeley and University of California, San Diego. He is best known for proposing the density wave theory to explain the structure of spiral galaxies, and for describing a model of star formation, where a giant dense molecular cloud collapses to form a star. molecular cloud collapses to form a star.
, 徐遐生（英語：Frank Hsia-San Shu，1943年6月2日－），籍貫浙江永嘉，出生于云南昆明，美籍華人天文學家，中央研究院院士。 其父親為徐賢修，父子皆曾任國立清華大學校長。
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فرانك شو
, Frank Shu
, Шу, Фрэнк
, 徐遐生
, フランク・シュー
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