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) |
|---|---|
| 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
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