Hostname: page-component-cd9895bd7-lnqnp Total loading time: 0 Render date: 2024-12-27T11:48:22.630Z Has data issue: false hasContentIssue false

Over 1000 Newly Discovered Young Stellar Objects in the Large Magellanic Cloud fromtheSpitzer SAGE Survey

Published online by Cambridge University Press:  13 November 2008

B.A. Whitney*
Affiliation:
Space Science Institute, 4750 Walnut St. Suite 205, Boulder, CO 80301, USA
Get access

Abstract

We have identified over 1000 candidate Young StellarObjects (YSOs) in the Large Magellanic Cloud as part of the Spitzer Space Telescope Surveying the Agents of a Galaxy's Evolution (SAGE) Legacy program. The YSOs, detected by their excess infrared emission above a stellar photosphere, representearly stages of evolution, still surrounded by disks and/or infalling envelopes.The candidate YSOs were selected from regions of color-magnitude space least confused with other IR-bright populations.Our YSO list is therefore biased towards intermediate- to high-mass and young evolutionarystages, because these overlap less with galaxies and evolved starsin color-magnitude space.We derived masses of the YSOs from SED-fitting, and extrapolated the mass function usinga standard IMF to compute a current star formation rate of ~0.06 M/yr, which is at the low-end ofestimates based on total ultraviolet and infrared flux from the galaxy (~0.05-0.25 M/yr); and consistent with the expectation that our current YSO list is incomplete.High spatial resolution K_dark- and L-band observations at Dome C could distinguish the lower-mass YSOs from galaxies, based on their morphologies(diffuse vs. point sources).This will add thousands more YSOs to our census and improve our estimates of star formationrate, molecular cloud lifetimes, and hierarchical star formation.In addition, the high spatial resolution Dome C observations can detect multiplicity in the SAGE-identified YSOs which can be incorporated into our YSO SED models.

Type
Research Article
Copyright
© EAS, EDP Sciences, 2008

Access options

Get access to the full version of this content by using one of the access options below. (Log in options will check for institutional or personal access. Content may require purchase if you do not have access.)

References

Bastian, N., Ercolano, B., Gieles, M., et al., 2007, MNRAS, 379, 1302 CrossRef
Bica, E., Claria, J.J., Dottori, H., Santos, J.F.C. Jr., & Piatti, A.E., 1996, ApJS, 102, 57 CrossRef
Blum, R.D., et al., 2006, AJ, 132, 2034 CrossRef
Calzetti, D., et al., 2007, ApJ, 666, 870 CrossRef
Carlson, L.R., et al., 2007, ApJ, 665, L109 CrossRef
Fazio, G.G., et al., 2004, ApJS, 154, 10 CrossRef
Fukui, Y., et al., 1999, PASJ, 51, 745
Gaustad, J.E., McCullough, P.R., Rosing, W., & Van Buren, D., 2001, PASP, 113, 1326 CrossRef
Hartmann, L., Ballesteros-Paredes, J., & Bergin, E.A., 2001, ApJ, 562, 852 CrossRef
Hora, J.L., et al., 2008, AJ, 135, 726 CrossRef
Kato, D., et al., 2007, PASJ, 59, 615 CrossRef
Kennicutt, R.C. Jr., 1998, ARA&A, 36, 189 CrossRef
Kroupa, P., 2001, MNRAS, 322, 231 CrossRef
Lonsdale, C., et al., 2004, ApJS, 154, 54 CrossRef
Meixner, M., et al., 2006, AJ, 132, 2268 CrossRef
Oestreicher, M.O., Gochermann, J., & Schmidt-Kaler, T., 1995, A&AS, 112, 495 PubMed
Panagia, N., 2005, in IAU Colloq. 192: Cosmic Explosions, On the 10th Anniversary of SN1993J, ed. J.-M., Marcaide, & K.W., Weiler (Berlin: Springer), p. 585
Rieke, G.H., et al., 2004, ApJS, 154, 25 CrossRef
Robitaille, T.P., Whitney, B.A., Indebetouw, R., Wood, K., & Denzmore, P., 2006, ApJS, 167, 256 CrossRef
Robitaille, T.P., Whitney, B.A., Indebetouw, R., & Wood, K., 2007, ApJS, 169, 328 CrossRef
Skrutskie, M.F., et al., 2006, AJ, 131, 1163 CrossRef
Smith, A.M., Cornett, R.H., & Hill, R.S., 1987, ApJ, 320, 609 CrossRef
Srinivasan, S., et al., 2008, AJ, submitted
van der Marel, R.P., & Cioni, M.-R.L., 2001, AJ, 122, 1807 CrossRef
Werner, M.W., et al., 2004, ApJS, 154, 1 CrossRef
Whitney, B.A., et al., 2008, AJ, in press