Hostname: page-component-cd9895bd7-dzt6s Total loading time: 0 Render date: 2024-12-25T17:02:14.232Z Has data issue: false hasContentIssue false
  • English
  • Français

VISTA variable survey in the Milky Way

Published online by Cambridge University Press:  13 April 2010

M. Hempel ,
D. Minniti ,
R. Saito ,
P. Pietrukowicz  and
P. W. Lucas
M. Hempel
Affiliation:
Pontificia Universidad Catolica de Chile, Departemento de Astronomie y Astrofisica, Av. Vic. Mackenna 4860, 7820436 Macul, Santiago, Chile email: [email protected], [email protected], [email protected], [email protected]
D. Minniti
Affiliation:
Pontificia Universidad Catolica de Chile, Departemento de Astronomie y Astrofisica, Av. Vic. Mackenna 4860, 7820436 Macul, Santiago, Chile email: [email protected], [email protected], [email protected], [email protected]
R. Saito
Affiliation:
Pontificia Universidad Catolica de Chile, Departemento de Astronomie y Astrofisica, Av. Vic. Mackenna 4860, 7820436 Macul, Santiago, Chile email: [email protected], [email protected], [email protected], [email protected]
P. Pietrukowicz
Affiliation:
Pontificia Universidad Catolica de Chile, Departemento de Astronomie y Astrofisica, Av. Vic. Mackenna 4860, 7820436 Macul, Santiago, Chile email: [email protected], [email protected], [email protected], [email protected]
P. W. Lucas
Affiliation:
Dept. of Astronomy, University of Hertfordshire, University of Hertfordshire, Hatfield AL10 9AB, UK email: [email protected]
Rights & Permissions [Opens in a new window]

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

Over the next 5 years the VVV collaboration (Vista Variable in the Via Lactea) will conduct an extensive survey of the galactic bulge and disk in the near-IR, using the new VISTA telescope. This public survey covers a field of 520 sqr. deg, including not only regions of high star formation, but also 33 known globular clusters and ~350 open clusters. The final product will be a deep IR atlas in 5 passbands for ~109 point sources among which we expect 106 variable stars. These will be produce a 3-D map of the surveyed region using well-understood primary distance indicators such as RR Lyrae stars. The observations will be combined with data from MACHO, OGLE, EROS, VST, Spitzer, HST, Chandra, Integral, and ALMA for a complete understanding of the variable sources in the inner Milky Way. Several important implications for the history of the Milky Way, for globular cluster evolution, for the population census of the bulge and center, and for the pulsation theory will follow from this survey.

Keywords

surveysstars: variables: Cepheidsstars: variables: otherGalaxy: bulgeGalaxy: disk
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 5 , Symposium S262: Stellar Populations – Planning for the Next Decade , August 2009 , pp. 287 - 290
Copyright
Copyright © International Astronomical Union 2010

References

Borissova, J., Pessev, P., Ivanov, V. D., et al. 2003, A&A, 411, 83Google Scholar
Carpenter, J. M., Hillenbrand, L. A., & Skrutskie, M. F. 2001, AJ, 121, 3160CrossRefGoogle Scholar
Catelan, M., Smith, H. A., Pritzl, B. J., et al. 2006, Mem. Soc. Astron. Italiana, 77, 202Google Scholar
Chanamé, J., Gould, A., & Miralda-Escudé, J. 2001, ApJ, 563, 793CrossRefGoogle Scholar
Ivanov, V. D., Borissova, J., Pessev, P., et al. 2002, A&A, 394, L1Google Scholar
Ivanov, V. D., Kurtev, R., & Borissova, J. 2005, A&A, 442, 195Google Scholar
Kerins, E., Robin, A. C., & Marshall, D. J. 2009, MNARS, 396, 1202CrossRefGoogle Scholar
Kuijken, K. & Rich, R. M. 2002, AJ, 124, 2054CrossRefGoogle Scholar
Meléndez, J., et al. 2008, A&A, 484, L21Google Scholar
Russell, D. M., Fender, R. P., Hynes, R. I., Brocksopp, C., Homan, J., Jonker, P. G., & Buxton, M. M. 2006, MNRAS 371, 1334CrossRefGoogle Scholar
Stanek, K. Z., Mateo, M., Udalski, A., et al. 1994, ApJL, 429, L73CrossRefGoogle Scholar
Zoccali, M., Renzini, A., Ortolani, S., et al. 2003, A&A, 399, 931Google Scholar
Zoccali, M., Lecureur, A., Barbuy, B., et al. 2006, A&A, 457, L1Google Scholar