Expected and observed late giant star counts in the Milky Way bulge
Author:
Publisher
Springer Science and Business Media LLC
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://link.springer.com/content/pdf/10.1007/BF00651149.pdf
Reference12 articles.
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3. de Vaucouleurs, G.: 1953,Monthly Notices Roy. Astron. Soc. 113, 134.
4. de Vaucouleurs, G. and Pence, W. D.: 1978,Astron. J. 83, 1163.
5. Hidayat, B. and Blanco, V. M.: 1968,Astron. J. 73, 712.
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1. MG II chromospheric-emission dating of HR 1614 moving-group stars;Publications of the Astronomical Society of the Pacific;1994-10
2. IRAS sources and the nature of the Galactic Bulge;Monthly Notices of the Royal Astronomical Society;1991-01-15
3. Kinematics and abundances of K giants in the nuclear bulge of the Galaxy;The Astrophysical Journal;1990-10
4. Galactic bulge M giants. III - Near-infrared spectra and implications for the stellar content of E and S0 galaxies;The Astrophysical Journal;1990-07
5. Mira Variables, Stellar Evolution and Galactic Structure;International Astronomical Union Colloquium;1989
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