<i>SPITZER</i>SURVEY OF THE LARGE MAGELLANIC CLOUD, SURVEYING THE AGENTS OF A GALAXY'S EVOLUTION (SAGE). IV. DUST PROPERTIES IN THE INTERSTELLAR MEDIUM

Bernard, Jean-Philippe; T. Reach, W.; Paradis, Déborah; Meixner, M.; Paladini, R.; Kawamura, Akiko; Onishi, Toshikazu; Vijh, U.; D. Gordon, Karl; Indebetouw, R.; L. Hora, Joseph; A. Whitney, B.; Blum, Robert; R. Meade, M.; Babler, B.; Churchwell, E.; W. Engelbracht, C.; For, Bi‐Qing; A. Misselt, K.; Leitherer, Claus; Cohen, Martin; Boulanger, F.; A. Frogel, J.; Fukui, Y.; S. Gallagher, J.; Gorjian, Varoujan; Harris, Jason; Kelly, Douglas; B. Latter, William; C. Madden, S.; Kemper, F.; Mizuno, Akira; Mizuno, N.; R. Mould, J.; Nota, A.; S. Oey, M.; Olsen, Knut; Panagia, N.; G. Pérez‐González, Pablo; Shibai, Hiroshi; Sato, Shuji; J. Smith, L.; Staveley‐Smith, L.; G. G. M. Tielens, A.; Ueta, Toshiya; D. Van Dyk, Schuyler; Volk, Kevin; W. Werner, M.; Zaritsky, Dennis

doi:10.1088/0004-6256/136/3/919

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SPITZERSURVEY OF THE LARGE MAGELLANIC CLOUD, SURVEYING THE AGENTS OF A GALAXY'S EVOLUTION (SAGE). IV. DUST PROPERTIES IN THE INTERSTELLAR MEDIUM

Shared by NobleBlocks on Jul 21, 2008 • 12:00 AM UTC

Authors:

Jean-Philippe Bernard

W. T. Reach

Déborah Paradis

Abstract

H i mass. We show that it is plausible that the FIR excess is due to cold atomic gas that is optically thick in the 21 cm line, while the contribution by a pure H 2 phase with no CO emission remains a possible explanation.

Subject

Physics

Astrophysics

Milky Way

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