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

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

Please use this identifier to cite or link to this item: http://hdl.handle.net/10355/5131

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dc.contributor.author Oliveira, J. M.
dc.contributor.author Loon, J. Th. van
dc.contributor.author Chen, C. H. R.
dc.contributor.author Tielens, A. G. G. M.
dc.contributor.author Sloan, G. C.
dc.contributor.author Woods, P. M.
dc.contributor.author Kemper, F.
dc.contributor.author Indebetouw, R.
dc.contributor.author Gordon, K. D.
dc.contributor.author Boyer, M. L.
dc.contributor.author Shiao, B.
dc.contributor.author Madden, S.
dc.contributor.author Speck, Angela K.
dc.contributor.author Meixner, Margaret
dc.contributor.author Marengo, M.
dc.date.accessioned 2010-01-27T20:02:02Z
dc.date.available 2010-01-27T20:02:02Z
dc.date.issued 2009-12-03
dc.identifier.citation The Astrophysical Journal, 707:1269-1295, 2009 December 20 en
dc.identifier.issn 1538-4357
dc.identifier.uri http://hdl.handle.net/10355/5131
dc.description http://www.iop.org/EJ/article/0004-637X/707/2/1269/apj_707_2_1269.pdf?request-id=762f8343-8c31-4613-a486-277ec46d1b8e en
dc.description.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 CO2 ice at 15.2 μm and the ice band between 5 and 7 μm that includes contributions from the bending mode of water ice at 6 μm among other ice species. The 5-7 μm band is difficult to identify in our LMC sample due to the conspicuous presence of polycyclic aromatic hydrocarbon 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 μm ice feature attributed in the literature to ammonium and methanol. We model the CO2 band in detail, using the combination of laboratory ice profiles available in the literature. We find that a significant fraction ( 50%) of CO2 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-CO2 contribution to the ice profile, evidence of thermal processing. There is a suggestion that CO2 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. en
dc.language.iso en_US en
dc.publisher American Astronomical Society en
dc.relation.ispartof Physics and Astronomy publications (MU) en
dc.source.uri http://www.iop.org/EJ/article/0004-637X/707/2/1269/apj_707_2_1269.pdf?request-id=762f8343-8c31-4613-a486-277ec46d1b8e en
dc.subject astrochemistry en
dc.subject galaxies en
dc.subject Magellanic clouds en
dc.subject.lcsh Cosmochemistry en
dc.subject.lcsh Circumstellar matter en
dc.subject.lcsh Magellanic Clouds en
dc.subject.lcsh Stars -- Formation en
dc.title Ice chemistry in embedded young stellar objects in the Large Magellanic Cloud en
dc.type Article en
dc.relation.ispartofcommunity University of Missouri-Columbia. College of Arts and Sciences. Department of Physics and Astronomy


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