Hostname: page-component-7bb8b95d7b-dvmhs Total loading time: 0 Render date: 2024-10-01T08:23:53.589Z Has data issue: false hasContentIssue false
  • English
  • Français

DIRECT Distances to Local Group Galaxies

Published online by Cambridge University Press:  12 April 2016

Dimitar D. Sasselov
Dimitar D. Sasselov*
Affiliation:
Harvard-Smithsonian Center for Astrophysics, 60 Garden St., Cambridge, MA 02138, USA

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.

The two nearby galaxies, M31 and M33, are stepping stones for most of our current efforts to understand the evolving universe at large scales. We are undertaking a long term project, called DIRECT, to improve the direct distance estimate to M31 and M33. The massive photometry we have obtained as part of our project over the past 3 years provides us with very good light curves for known and new Cepheid variables, a large number of eclipsing binaries and other variable stars.

Type
Part 3. Cepheids, RR Lyrae Stars, Distance Scales
Information
International Astronomical Union Colloquium , Volume 176: The Impact of Large-Scale Surveys on Pulsating Star Research , 2000 , pp. 182 - 186
Copyright
Copyright © Astronomical Society of the Pacific 2000

References

Aparicio, A., Herrero, A., & Sanchez, F. (ed.) 1998, Stellar Astrophysics for the Local Group, VIII Can. Isl. Winter School (New York: CUP)Google Scholar
Beaulieu, J.P. & Sasselov, D. 1997, in Variable Stars and the Astrophysical Returns of the Microlensing Surveys, ed. Ferlet, R., Maillard, J.-P., & Raban, B. (Gif-sur-Yvette: Editions Frontières), 193 Google Scholar
Buchler, J.R. 1997, in Variable Stars and the Astrophysical Returns of the Microlensing Surveys, ed. Ferlet, R., Maillard, J.-P., & Raban, B. (Gif-sur-Yvette: Editions Frontières), 181 Google Scholar
Holland, S. 1998, AJ, 115, 1916 Google Scholar
Huterer, D., Sasselov, D., & Schechter, P. 1995, AJ, 100, 2705 CrossRefGoogle Scholar
Kaluzny, J., Stanek, K., Krockenberger, M., Sasselov, D., et al. 1998, AJ, 115, 1016 Google Scholar
Kaluzny, J., Mochejska, B., Stanek, K., et al. 1999, AJ, 118, 346 Google Scholar
Mochejska, B., Macri, L., Sasselov, D., & Stanek, K. 1999, AJ, submitted [astro- ph/9908293]Google Scholar
Mould, J., Huchra, J., Freedman, W., et al. 1999, preprint [astro-ph/9909260]Google Scholar
Stanek, K. & Garnavich, P. 1998, ApJ, 503, L131 Google Scholar
Stanek, K., Kaluzny, J., Krockenberger, M., et al. 1998, AJ, 115, 1894 Google Scholar
Stanek, K., Kaluzny, J., Krockenberger, M., Sasselov, D., et al. 1999, AJ, 117, 2810 CrossRefGoogle Scholar