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- W3100696356 abstract "VDB0-B195D is a massive, blue star cluster in M31. It was observed as part of the Beijing-Arizona-Taiwan-Connecticut (BATC) Multicolor Sky Survey using 15 intermediate-band filters covering a wavelength range of 3000--10,000 AA. Based on aperture photometry, we obtain its spectral-energy distribution (SED) as defined by the 15 BATC filters. We apply previously established relations between the BATC intermediate-band and the Johnson-Cousins $UBVRI$ broad-band systems to convert our BATC photometry to the standard system. A detailed comparison shows that our newly derived $VRI$ magnitudes are fully consistent with previous results, while our new $B$ magnitude agrees to within $2sigma$. In addition, we determine the cluster's age and mass by comparing its SED (from 3000 to 20,000{AA}, comprising photometric data in the 15 BATC intermediate bands, optical broad-band $BVRI$, and 2MASS near-infrared $JHK_{rm s}$ data) with theoretical stellar population synthesis models, resulting in age and mass determinations of $60.0pm 8.0$~Myr and $(1.1-1.6) times 10^5 M_odot$, respectively. This age and mass confirms previous suggestions that VDB0-B195D is a young massive cluster in M31." @default.
- W3100696356 created "2020-11-23" @default.
- W3100696356 creator A5000289914 @default.
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- W3100696356 date "2011-02-04" @default.
- W3100696356 modified "2023-10-16" @default.
- W3100696356 title "AGE AND MASS CONSTRAINTS FOR A YOUNG MASSIVE CLUSTER IN M31 BASED ON SPECTRAL ENERGY DISTRIBUTION FITTING" @default.
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