The Shortest-Known―Period Star Orbiting Our Galaxy's Supermassive Black Hole
- Author
- MEYER, L1 ; GHEZ, A. M1 ; SCHÖDEL, R2 ; YELDA, S1 ; BOEHLE, A1 ; LU, J. R3 ; DO, T4 5 ; MORRIS, M. R1 ; BECKLIN, E. E1 ; MATTHEWS, K6
[1] Department of Physics and Astronomy, University of California Los Angeles, Los Angeles, CA 90095-1547, United States
[2] Instituto de Astrofísica de Andalucía (CSIC), Glorieta de la Astronomia S/N, 18008 Granada, Spain
[3] Institute for Astronomy, University of Hawaii, Honolulu, HI 96822, United States
[4] Department of Physics and Astronomy, University of California Irvine, Irvine, CA 92697-4575, United States
[5] Dunlap Institute for Astronomy and Astrophysics, University of Toronto, Toronto M5S 3H4, Ontario, Canada
[6] Division of Mathematics, Physics and Astronomy, California Institute of Technology, Pasadena, CA 91125, United States - Source
Science (Washington, D.C.). 2012, Vol 338, Num 6103, pp 84-87, 4 p
- CODEN
- SCIEAS
- ISSN
- 0036-8075
- Scientific domain
- Multidisciplinary
- Publisher
- American Association for the Advancement of Science, Washington, DC
- Publication country
- United States
- Document type
- Article
- Language
- English
- Keyword (fr)
- Centre galactique Cosmologie Dégénérescence Potentiel central Potentiel gravitationnel Relativité générale Théorie Einstein Trou noir supermassif Voie lactée
- Keyword (en)
- Galactic centers Cosmology Degeneration Central potential Gravitational potential General relativity Einstein theory Supermassive black hole Milky Way
- Keyword (es)
- Teoría Einstein Agujero negro supermasivo
- Classification
- Pascal
- 001 Exact sciences and technology / 001E Earth, ocean, space / 001E03 Astronomy / 001E03D Stellar systems. Galactic and extragalactic objects and systems. The universe / 001E03D35 Characteristics and properties of the milky way / 001E03D35J Galactic center, bar, circumnuclear matter, and bulge (including black hole and distance measurements)
- Discipline
- Astronomy
- Origin
- Inist-CNRS
- Database
- PASCAL
- INIST identifier
- 26691253
Sauf mention contraire ci-dessus, le contenu de cette notice bibliographique peut être utilisé dans le cadre d’une licence CC BY 4.0 Inist-CNRS / Unless otherwise stated above, the content of this bibliographic record may be used under a CC BY 4.0 licence by Inist-CNRS / A menos que se haya señalado antes, el contenido de este registro bibliográfico puede ser utilizado al amparo de una licencia CC BY 4.0 Inist-CNRS
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DOI
10.1126/science.1225506 
https://dx.doi.org/10.1126/science.1225506
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