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Ice chemistry in embedded young stellar objects in the Large Magellanic Cloud

Oliveira, J. M.; van Loon, J. Th.; Chen, C.-H. R.; Tielens, A. G. G. M.; Sloan, G. C.; Woods, P. M.; Kemper, F.; Indebetouw, R.; Gordon, K. D.; Boyer, M. L.; Shiao, B.; Madden, S.; Speck, A. K.; Meixner, M.; Marengo, M.

Authors

C.-H. R. Chen

A. G. G. M. Tielens

G. C. Sloan

P. M. Woods

F. Kemper

R. Indebetouw

K. D. Gordon

M. L. Boyer

B. Shiao

S. Madden

A. K. Speck

M. Meixner

M. Marengo



Abstract

We present spectroscopic observations of a sample of 15 embedded young stellar objects (YSOs) in the Large Magellanic Cloud (LMC). These observations were obtained with the Spitzer Infrared Spectrograph (IRS) as part of the SAGE-Spec Legacy program. We analyze the two prominent ice bands in the IRS spectral range: the bending mode of CO_2 ice at 15.2 micron and the ice band between 5 and 7 micron that includes contributions from the bending mode of water ice at 6 micron amongst other ice species. The 5-7 micron band is difficult to identify in our LMC sample due to the conspicuous presence of PAH emission superimposed onto the ice spectra. We identify water ice in the spectra of two sources; the spectrum of one of those sources also exhibits the 6.8 micron ice feature attributed to ammonium and methanol. We model the CO_2 band in detail, using the combination of laboratory ice profiles available in the literature. We find that a significant fraction (> 50%) of CO_2 ice is locked in a water-rich component, consistent with what is observed for Galactic sources. The majority of the sources in the LMC also require a pure-CO_2 contribution to the ice profile, evidence of thermal processing. There is a suggestion that CO_2 production might be enhanced in the LMC, but the size of the available sample precludes firmer conclusions. We place our results in the context of the star formation environment in the LMC.

Citation

Oliveira, J. M., van Loon, J. T., Chen, C. R., Tielens, A. G. G. M., Sloan, G. C., Woods, P. M., …Marengo, M. (2009). Ice chemistry in embedded young stellar objects in the Large Magellanic Cloud. Astrophysical Journal, 707(1269), https://doi.org/10.1088/0004-637X/707/2/1269

Journal Article Type Article
Acceptance Date Nov 4, 2009
Online Publication Date Nov 3, 2009
Publication Date Nov 3, 2009
Deposit Date Jul 6, 2023
Publicly Available Date Jul 6, 2023
Journal Astrophys.J.707:1269-1295,2009
Print ISSN 0004-637X
Publisher American Astronomical Society
Peer Reviewed Peer Reviewed
Volume 707
Issue 1269
DOI https://doi.org/10.1088/0004-637X/707/2/1269
Keywords Solar and Stellar Astrophysics; Astrophysics of Galaxies; astrochemistry – circumstellar matter – galaxies: individual (LMC) – Magellanic Clouds – stars: formation