Three classical Cepheid variable stars in the nuclear bulge of the Milky Way-Reference-Cited by-同舟云学术

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Three classical Cepheid variable stars in the nuclear bulge of the Milky Way

Published:2011-08-24 Issue:7363 Volume:477 Page:188-190
ISSN:0028-0836
Container-title:Nature
language:en
Short-container-title:Nature

Author:

Matsunaga Noriyuki,Kawadu Takahiro,Nishiyama Shogo,Nagayama Takahiro,Kobayashi Naoto,Tamura Motohide,Bono Giuseppe,Feast Michael W.,Nagata Tetsuya

Publisher

Springer Science and Business Media LLC

Subject

Multidisciplinary

Link

http://www.nature.com/articles/nature10359.pdf

Reference26 articles.

1. Launhardt, R., Zylka, R. & Mezger, P. G. The nuclear bulge of the Galaxy. III. Large-scale physical characteristics of stars and interstellar matter. Astron. Astrophys. 384, 112–139 (2002)

2. Serabyn, E. & Morris, M. Sustained star formation in the central stellar cluster of the Milky Way. Nature 382, 602–604 (1996)

3. van Loon, J. Th. et al. Infrared stellar populations in the central parts of the Milky Way galaxy. Mon. Not. R. Astron. Soc. 338, 857–879 (2003)

4. Figer, D. F., Rich, R. M., Kim, S. S., Morris, M. & Serabyn, E. An extended star formation history for the Galactic Center from Hubble Space Telescope NICMOS observations. Astrophys. J. 601, 319–339 (2004)

5. Yusef-Zadeh, F. et al. Star formation in the central 400 pc of the Milky Way: Evidence for a population of massive young stellar objects. Astrophys. J. 702, 178–225 (2009)

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