Journal article
STAR FORMATION IN THE CENTRAL 400 PC OF THE MILKY WAY: EVIDENCE FOR A POPULATION OF MASSIVE YOUNG STELLAR OBJECTS
The Astrophysical journal, Vol.702(1), pp.178-225
09/01/2009
DOI: 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 mu m 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 mu m excesses. We use the SEDs of these sources to estimate their physical characteristics; their masses appear to range from similar to 10 to similar to 20 M-circle dot. Within the central 400 x 50 pc (vertical bar l vertical bar < 1 degrees.3 and vertical bar b vertical bar < 10') the star formation rate (SFR) based on the identification of Stage I evolutionary phase of YSO candidates is about 0.14 M-circle dot 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 10(5) yr. This suggestion is also consistent with estimates of SFRs within the last similar to 10(7) yr showing a peak around 10(5) 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.
Details
- Title: Subtitle
- STAR FORMATION IN THE CENTRAL 400 PC OF THE MILKY WAY: EVIDENCE FOR A POPULATION OF MASSIVE YOUNG STELLAR OBJECTS
- Creators
- F. Yusef-Zadeh - Northwestern UniversityJ. W. Hewitt - Northwestern UniversityR. G. Arendt - NASA, Goddard Space Flight Ctr, Sci Syst & Applicat Inc, Greenbelt, MD 20771 USAB. Whitney - Space Sci Inst, Boulder, CO 80301 USAG. Rieke - University of ArizonaM. Wardle - Macquarie UniversityJ. L. Hinz - University of ArizonaS. Stolovy - California Institute of TechnologyC. C. Lang - Univ Iowa, Dept Phys & Astron, Iowa City, IA 52245 USAM. G. Burton - Univ New S Wales, Sch Phys, Sydney, NSW 2052, AustraliaS. Ramirez - California Institute of Technology
- Resource Type
- Journal article
- Publication Details
- The Astrophysical journal, Vol.702(1), pp.178-225
- DOI
- 10.1088/0004-637X/702/1/178
- ISSN
- 0004-637X
- eISSN
- 1538-4357
- Publisher
- Iop Publishing Ltd
- Number of pages
- 48
- Language
- English
- Date published
- 09/01/2009
- Academic Unit
- Liberal Arts and Science Admin; Physics and Astronomy
- Record Identifier
- 9984428793402771
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