STAR FORMATION IN THE CENTRAL 400 PC OF THE MILKY WAY: EVIDENCE FOR A POPULATION OF MASSIVE YOUNG STELLAR OBJECTS
Open Access
- 10 August 2009
- journal article
- Published by American Astronomical Society in The Astrophysical Journal
- Vol. 702 (1), 178-225
- https://doi.org/10.1088/0004-637x/702/1/178
Abstract
The central kpc of the Milky Way might be expected to differ significantly from the rest of the Galaxy with regard to gasdynamics and the formation of young stellar objects (YSOs). We probe this possibility with mid-infrared observations obtained with Infrared Array Camera and Multiband Imaging Photometer on Spitzer and with Midcourse Space Experiment. We use color-color diagrams and spectral energy distribution (SED) fits to explore the nature of YSO candidates (including objects with 4.5 μm excesses possibly due to molecular emission). There is an asymmetry in the distribution of the candidate YSOs, which tend to be found at negative Galactic longitudes; this behavior contrasts with that of the molecular gas, approximately 2/3 of which is at positive longitudes. The small-scale height of these objects suggests that they are within the Galactic center region and are dynamically young. They lie between two layers of infrared dark clouds and may have originated from these clouds. We identify new sites for this recent star formation by comparing the mid-IR, radio, submillimeter, and methanol maser data. The methanol masers appear to be associated with young, embedded YSOs characterized by 4.5 μm excesses. We use the SEDs of these sources to estimate their physical characteristics; their masses appear to range from ~10 to ~20 M ☉. Within the central 400 × 50 pc (|l| < 13 and |b| < 10') the star formation rate (SFR) based on the identification of Stage I evolutionary phase of YSO candidates is about 0.14 M ☉ yr–1. Given that the majority of the sources in the population of YSOs are classified as Stage I objects, we suggest that a recent burst of star formation took place within the last 105 yr. This suggestion is also consistent with estimates of SFRs within the last ~107 yr showing a peak around 105 yr ago. Lastly, we find that the Schmidt-Kennicutt Law applies well in the central 400 pc of the Galaxy. This implies that star formation does not appear to be dramatically affected by the extreme physical conditions in the Galactic center region.Keywords
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This publication has 100 references indexed in Scilit:
- STAR FORMATION ACTIVITY OF CORES WITHIN INFRARED DARK CLOUDSThe Astrophysical Journal Supplement Series, 2009
- THE MID-INFRARED EXTINCTION LAW IN THE OPHIUCHUS, PERSEUS, AND SERPENS MOLECULAR CLOUDSThe Astrophysical Journal, 2008
- The Origin of Diffuse X‐Ray and γ‐Ray Emission from the Galactic Center Region: Cosmic‐Ray ParticlesThe Astrophysical Journal, 2007
- The Characterization and Galactic Distribution of Infrared Dark CloudsThe Astrophysical Journal, 2006
- A mid-infrared survey of the inner 2 × 1.5 degrees of the Galaxy with Spitzer/IRACJournal of Physics: Conference Series, 2006
- Hot and Diffuse Clouds near the Galactic Center Probed by Metastable H3+* ** ***The Astrophysical Journal, 2005
- ISOGAL: A deep survey of the obscured inner Milky Way with ISO at 7 μm and 15 μm and with DENIS in the near-infraredAstronomy & Astrophysics, 2003
- Submillimeter Observations of [ITAL]Midcourse Space Experiment[/ITAL] Galactic Infrared-Dark CloudsThe Astrophysical Journal, 2000
- Hubble Space Telescope/NICMOS Observations of Massive Stellar Clusters near the Galactic CenterThe Astrophysical Journal, 1999
- Galactic center molecular clouds. II - Distribution and kinematicsThe Astrophysical Journal, 1988