The Color--Magnitude Diagram in Baade's Window Revisited
arXiv:astro-ph/9608169 · doi:10.1086/304441
Abstract
We have reanalyzed the OGLE and photometry of stars in Baade's Window, and we confirm the extinction map published by Stanek (1996). However, we find that the interpretation of the OGLE color--magnitude diagram for the disk stars proposed by Paczyński et al. (1994) was incorrect: the dominant disk population in Baade's Window is old, and we find no evidence for a large hole in the inner Galactic disk. We find evidence for a small systematic error in the OGLE photometry for stars below the ``red clump'': the faint stars with have their color indices too red by . We find tentative evidence from the OGLE and HST photometry that the the bulge main sequence turn--off point is brighter by than it is in either 47~Tuc or NGC~6791, indicating that the dominant population of the Galactic bulge is considerably younger than those clusters.
arXiv commentsubmitted to the Astrophysical Journal, 17 pages, 9 figures, 4 figures included; all figures are available using ftp://www.astro.princeton.edu/stanek/Kiraga
References in corpus (5)
- Modelling the Galactic Bar Using Red Clump Giants
- Color-Magnitude Diagram Distribution of the Bulge Red Clump Stars - Evidence for the Galactic Bar
- Extinction Map of Baade's Window
- The Distribution of Galactic Disk Stars in Baade's Window
- Variations of the Selective Extinction Across the Galactic Bulge - Implications for the Galactic Bar
Cited by in corpus (16)
- Reddening and Extinction Toward the Galactic Bulge from OGLE-III: The Inner Milky Way's Rv ~ 2.5 Extinction Curve
- Distances, ages, and epoch of formation of globular clusters
- Distance to M31 With the HST and Hipparcos Red Clump Stars
- Galactocentric Distance With the OGLE and Hipparcos Red Clump Stars
- Extinction Map of the Galactic center: OGLE-II Galactic bulge fields
- Microlensing of Blended Stellar Images
- The Microlensing Event Rate and Optical Depth Toward the Galactic Bulge from MOA-II
- Possible Solution of the long-standing discrepancy in the Microlensing Optical Depth Toward the Galactic Bulge by correcting the stellar number count
- Evidence for a deficit of young and old stars in the Milky Way inner in-plane disc
- The Large-Scale Extinction Map of the Galactic Bulge from the MACHO Project Photometry
- Eclipsing Binaries in the OGLE Variable Star Catalog.III. Long-Period Contact Systems
- Mapping the Interstellar Reddening and Extinction towards Baade's Window Using Minimum Light Colors of ab-type RR Lyrae Stars. Revelations from the De-reddened Color-Magnitude Diagrams
- A Near-Infrared Photometric Survey of Metal-Poor Inner Spheroid Globular Clusters and Nearby Bulge Fields
- 8-13um Dust Emission Features in Galactic Bulge Planetary Nebulae
- Eclipsing Binaries in the OGLE Variable Star Catalog. IV. The Pre-Contact, Equal-Mass Systems
- A Survey for EHB Stars in the Galactic Bulge