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Cited article:
H. S. Liszt , J. Pety , R. Lucas
A&A, 518 (2010) A45
Published online: 2010-09-01
This article has been cited by the following article(s):
112 articles | Pages:
THE ABUNDANCE OF C
3
H
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AND OTHER SMALL HYDROCARBONS IN THE DIFFUSE INTERSTELLAR MEDIUM
Harvey Liszt, Paule Sonnentrucker, Martin Cordiner and Maryvonne Gerin The Astrophysical Journal 753 (2) L28 (2012) https://doi.org/10.1088/2041-8205/753/2/L28
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A. V. Kasparova Astronomy Letters 38 (2) 63 (2012) https://doi.org/10.1134/S1063773712020041
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H. S. Liszt Astronomy & Astrophysics 538 A27 (2012) https://doi.org/10.1051/0004-6361/201117882
Residual cooling and persistent star formation amid active galactic nucleus feedback in Abell 2597
G. R. Tremblay, C. P. O’Dea, S. A. Baum, et al. Monthly Notices of the Royal Astronomical Society 424 (2) 1042 (2012) https://doi.org/10.1111/j.1365-2966.2012.21278.x
SPITZERINFRARED SPECTROGRAPH DETECTION OF MOLECULAR HYDROGEN ROTATIONAL EMISSION TOWARDS TRANSLUCENT CLOUDS
James G. Ingalls, T. M. Bania, F. Boulanger, et al. The Astrophysical Journal 743 (2) 174 (2011) https://doi.org/10.1088/0004-637X/743/2/174
THE FAR-ULTRAVIOLET “CONTINUUM” IN PROTOPLANETARY DISK SYSTEMS. II. CARBON MONOXIDE FOURTH POSITIVE EMISSION AND ABSORPTION*
Kevin France, Rebecca N. Schindhelm, Eric B. Burgh, et al. The Astrophysical Journal 734 (1) 31 (2011) https://doi.org/10.1088/0004-637X/734/1/31
The CO-H2 conversion factor in disc galaxies and mergers
Desika Narayanan, Mark Krumholz, Eve C. Ostriker and Lars Hernquist Monthly Notices of the Royal Astronomical Society 418 (1) 664 (2011) https://doi.org/10.1111/j.1365-2966.2011.19516.x
How does C+recombine in diffuse molecular gas?
H. S. Liszt Astronomy & Astrophysics 527 A45 (2011) https://doi.org/10.1051/0004-6361/201015824
Modelling CO emission - I. CO as a column density tracer and the X factor in molecular clouds
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THE CO-TO-H2CONVERSION FACTOR FROM INFRARED DUST EMISSION ACROSS THE LOCAL GROUP
Adam K. Leroy, Alberto Bolatto, Karl Gordon, et al. The Astrophysical Journal 737 (1) 12 (2011) https://doi.org/10.1088/0004-637X/737/1/12
The CO-H2conversion factor of diffuse ISM: Bright12CO emission also traces diffuse gas
J. Pety, H.S. Liszt and R. Lucas EAS Publications Series 52 151 (2011) https://doi.org/10.1051/eas/1152024
Modelling CO emission - II. The physical characteristics that determine the X factor in Galactic molecular clouds
Rahul Shetty, Simon C. Glover, Cornelis P. Dullemond, et al. Monthly Notices of the Royal Astronomical Society 415 (4) 3253 (2011) https://doi.org/10.1111/j.1365-2966.2011.18937.x
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