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2001AJ....121.2020B - Astron. J., 121, 2020-2031 (2001/April-0)
The massive star content of NGC 6822: ground-based and Hubble space telescope photometry.
BIANCHI L., SCUDERI S., MASSEY P. and ROMANIELLO M.
Abstract (from CDS):
The luminosity function for the UV-selected stars in the two WFPC2 fields shows two components: a population with age of a few million years in the regions of Hubble V and Hubble X, and a 10 million year old background population. The main-sequence stellar luminosity function, including all stars measured in the V filter, is similar to the canonical composite luminosity function for main-sequence Galactic field stars.
The reddening (foreground plus internal) is found to vary between E(B-V)=0.25 and 0.45.
Abstract Copyright: ∼
Journal keyword(s): Galaxies: Individual: NGC Number: NGC 6822 - Galaxies: Stellar Content - Galaxies: Local Group - Stars: Formation - Stars: Luminosity Function, Mass Function - Stars: Color-Magnitude Diagrams
VizieR on-line data: <Available at CDS (J/AJ/121/2020): table1.dat table3.dat>
Nomenclature: Table 1: [BSM2001] CTIO-NNNN (Nos 1-3232). Table 3: [BSM2001] LB-f1-NNN N=760, [BSM2001] LB-f2-NNN N=260.
Simbad objects: 367
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