Hostname: page-component-586b7cd67f-2plfb Total loading time: 0 Render date: 2024-11-26T22:29:36.593Z Has data issue: false hasContentIssue false
  • English
  • Français

Direct DEBs in M31 and M33

Published online by Cambridge University Press:  30 March 2016

Lucas M. Macri
Lucas M. Macri*
Affiliation:
Hubble Fellow, National Optical Astronomy Observatory, 950 N Cherry Avenue, Tucson, AZ 85719, USA

Extract

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 DIRECT project (as in “direct distances”) started in 1996 with the long-term goal of obtaining distances to two important galaxies in the cosmological distance ladder – M31 and M33 – using detached eclipsing binaries (DEBs) and Cepheids. These two nearby galaxies are the stepping stones in most of the current effort to understand the evolving universe at large scales. Not only are they essential to the calibration of the extragalactic distance scale, but they also constrain population synthesis models for early galaxy formation and evolution. However, accurate distances are essential to make these calibrations free from large systematic uncertainties.

Type
I. Joint Discussions
Information
Highlights of Astronomy , Volume 13 , 2005 , pp. 452 - 453
Copyright
Copyright © Astronomical Society of Pacific 2005

References

Bonanos, A. Z., Stanek, K. Z., Sasselov, D. D., Mochejska, B. J., Macri, L. M., & Kaluzny, J. 2003, AJ, 126, 175 CrossRefGoogle Scholar
Fitzpatrick, E. L., Ribas, I., Guinan, E. F., Maloney, F. P., & Claret, A. 2003, ApJ, 587, 685 CrossRefGoogle Scholar
Kaluzny, J., Stanek, K. Z., Krockenberger, M., Sasselov, D. D., Tonry, J. L., & Mateo, M. 1998, AJ, 115, 1016 CrossRefGoogle Scholar
Kaluzny, J., Mochejska, B. J., Stanek, K. Z., Krockenberger, M., Sasselov, D. D., Tonry, J. L., & Mateo, M. 1999, AJ, 188, 346 Google Scholar
Macri, L. M., Sasselov, D. D. & Stanek, K. Z. 2001a, ApJ, 550, L159 Google Scholar
Macri, L. M., Stanek, K. Z., Sasselov, D. D., Krockenberger, M., & Kaluzny, J. 2001b, AJ, 120, 861 CrossRefGoogle Scholar
Macri, L. M., Stanek, K. Z., Sasselov, D. D., Krockenberger, M., & Kaluzny, J. 2001c, AJ, 120, 870 CrossRefGoogle Scholar
Mochejska, B. J., Kaluzny, J., Krockenberger, M., Sasselov, D. D., & Stanek, K. Z. 1998, AcA, 48, 445 Google Scholar
Mochejska, B. J., Kaluzny, J., Stanek, K. Z., Krockenberger, M., & Sasselov, D. D. 1999, AJ, 118, 2211 CrossRefGoogle Scholar
Mochejska, B. J., Macri, L. M., Sasselov, D. D., & Stanek, K. Z. 2000, AJ, 120, 810 Google Scholar
Mochejska, B. J., Macri, L. M., Sasselov, D. D., & Stanek, K. Z. 2001a, astro-ph/0103440 Google Scholar
Mochejska, B. J., Kaluzny, J., Stanek, K. Z., & Sasselov, D. D. 2001b, AJ, 122, 1383 CrossRefGoogle Scholar
Mochejska, B. J., Kaluzny, J., Stanek, K. Z., Sasselov, D. D., & Szentgyorgyi, A. H. 2001c, AJ, 121, 2032 Google Scholar
Mochejska, B. J., Kaluzny, J., Stanek, K. Z., Sasselov, D. D., & Szentgyorgyi, A. H. 2001d, AJ, 122, 2477 CrossRefGoogle Scholar
Paczyński, B. 1997, in The Extragalactic Distance Scale, ed. Livio, M., Donahue, M. & Panagia, N. (Cambridge: Cambridge Univ. Press), 273 Google Scholar
Stanek, K. Z., Kaluzny, J., Krockenberger, M., Sasselov, D. D., Tonry, J. L., & Mateo, M. 1998, AJ, 115, 1894 Google Scholar
Stanek, K. Z., Kaluzny, J., Krockenberger, M., Sasselov, D. D., Tonry, J. L., & Mateo, M. 1999, AJ, 117, 2810 Google Scholar