Abstract
The V838 Mon's behavior and the nature of the progenitor object are not well understood. Type B stars recently have been found in the vicinity of V838 Mon and it is thought that they may be part of a young open cluster. Since the cluster is in a spiral arm of the Galaxy, the identification of additional member stars is complicated; therefore, photometric and spectroscopic studies are necessary. We present the preliminary results of our photometric analyses with images obtained from the Advanced Camera for Surveys (ACS) on Hubble Space Telescope (HST).
Original language | English (US) |
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Pages (from-to) | 135-136 |
Number of pages | 2 |
Journal | Revista Mexicana de Astronomia y Astrofisica: Serie de Conferencias |
Volume | 34 |
State | Published - 2008 |
Event | IV Reunion Sobre Astronomia Dinamica en Latinoamerica, ADeLA-2008 - Mexico, D.F., Mexico Duration: Feb 12 2008 → Feb 16 2008 |
All Science Journal Classification (ASJC) codes
- Space and Planetary Science
- Astronomy and Astrophysics