CHAMP+ observations of warm gas in M 17 SW
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Leiden Observatory | A. Baryshev | M. R. Hogerheijde | M. Spaans | M. F. Astronomy | L. Observatory | A. Baryshev | M. Hogerheijde | Sron Netherlands Institute for Space Research | J. P. P'erez-Beaupuits | M. Spaans | R.Gusten | W. Boland Kapteyn Astronomical Institute | Max-Planck Institute for Radio Astronomy | SRON Netherlands Institute for Space Research | NOVA Nederlandse Onderzoeksschool Voor Astronomie | J. P'erez-Beaupuits | W. Institute | Nova Nederlandse Onderzoeksschool Voor Astronomie | S. I. F. S. Research
[1] C. Lada. Detailed observations of the M17 molecular cloud complex , 1976 .
[2] I. Gatley,et al. The appearance of dusty H II blisters at radio and infrared wavelengths , 1980 .
[3] P. J. Huggins,et al. Temperatures of galactic molecular clouds showing CO self-absorption , 1981 .
[4] L. Mundy,et al. Models of molecular clouds. I. Multitransition study of CS. , 1984 .
[5] R. Hills,et al. CO emission from fragmentary molecular clouds: a model applied to observations of M17 SW , 1984 .
[6] P. J. Huggins,et al. The abundance of atomic carbon near the ionization fronts in M17 and S140 , 1985 .
[7] E. I. Robson,et al. Submillimeter and millimeter observations of jupiter , 1986 .
[8] Robert N. Martin,et al. Submillimeter Observations of CS in M17 , 1986 .
[9] L. Mundy,et al. Submillimeter spectral line observations in very dense regions , 1987 .
[10] R. Genzel,et al. Warm dense gas in luminous protostellar regions - a submillimeter and far-infrared CO line study , 1987 .
[11] J. Stutzki,et al. Submillimeter and Far-Infrared Spectroscopy of M17 and S106: UV-heated, Quiescent Molecular Gas? , 1987 .
[12] Gordon J. Stacey,et al. Submillimeter and far-infrared line observations of M17 SW - A clumpy molecular cloud penetrated by ultraviolet radiation , 1988 .
[13] J. Stutzki,et al. High spatial resolution observations of neutral atomic carbon in the molecular clouds M17 and W51 , 1988 .
[14] J. Stutzki,et al. High spatial resolution isotopic CO and CS observations of M17 SW - The clumpy structure of the molecular cloud core , 1989 .
[15] A. Penzias,et al. C-12/C-13 isotope ratio across the Galaxy from observations of C-13/O-18 in molecular clouds , 1990 .
[16] A. Tielens,et al. Far-infrared observations of M17SW - The clumpy structure of the photodissociation region , 1992 .
[17] N. Evans,et al. Structure of Dense Cores in M17 SW. I. A Multitransition CS and C 34S Study , 1993 .
[18] A. Poglitsch,et al. CO Lines toward NGC 2024 and Other Star-forming Regions: A Closer Look at the Warm Gas Component , 1993 .
[19] E. Bergin,et al. CH3C2H AS A TEMPERATURE PROBE IN DENSE GIANT MOLECULAR CLOUD CORES , 1994 .
[20] E. Bergin,et al. Density Structure in Giant Molecular Cloud Cores , 1996 .
[21] I. Howarth,et al. The Young Massive Stellar Objects of M17 , 1997 .
[22] M. Gerin,et al. Atomic Carbon in Arp 220 , 1998 .
[23] NASA Ames Research Center,et al. Far-Infrared and Submillimeter Emission from Galactic and Extragalactic Photodissociation Regions , 1999, astro-ph/9907255.
[24] C. Wilson,et al. The Large-Scale J = 3 → 2 and J = 2 → 1 CO Emission from M17 and Its Implications for Extragalactic CO Observations , 1999, astro-ph/9901134.
[25] Charles L. Bennett,et al. COBE Far Infrared Absolute Spectrophotometer Observations of Galactic Lines , 1999 .
[26] M. Harwit,et al. The Distribution of Water Emission in M17SW , 2000, astro-ph/0010392.
[27] M. Harwit,et al. Extended [C [CSC]i[/CSC]] and [TSUP]13[/TSUP]CO (5 → 4) Emission in M17SW , 2000 .
[28] C. Brogan,et al. VLA H I and OH Zeeman Observations toward M17 , 2001 .
[29] H. Maezawa,et al. Observation of the C I 3P2-3P1 Line toward the Orion Kleinmann-Low Region , 2001 .
[30] C. Kramer,et al. A multiwavelength study of the S106 region I. Structure and dynamics of the molecular gas , 2002 .
[31] Mapping of large scale 158 [CII] line emission: orion A , 2003, astro-ph/0304242.
[32] C. Kramer,et al. A multiwavelength study of the S 106 region II. Characteristics of the photon dominated region , 2003 .
[33] A. Weiss,et al. Gas and dust in the Cloverleaf quasar at redshift 2.5 , 2003, astro-ph/0309048.
[34] C. Kramer,et al. Emission of CO, C i, and C ii in W3 Main , 2004, astro-ph/0406141.
[35] Diagnostics of irradiated gas in galaxy nuclei. I. A far-ultraviolet and X-ray dominated region code , 2005, astro-ph/0502454.
[36] J. Black,et al. An atomic and molecular database for analysis of submillimetre line observations , 2004, astro-ph/0411110.
[37] Photon dominated regions in the spiral arms of M 83 and M 51 , 2005, astro-ph/0505627.
[38] M. Spaans,et al. THE EXCITATION OF WATER IN THE S140 PHOTON DOMINATED REGION. D. R. Poelman , 2005, astro-ph/0506111.
[39] P. Jankowski,et al. Improved low-temperature rate constants for rotational excitation of CO by H 2 , 2006, astro-ph/0601384.
[40] A. Belloche,et al. APECS : the Atacama pathfinder experiment control system , 2006 .
[41] A survey of submillimeter C and CO lines in nearby galaxies , 2006, astro-ph/0611340.
[42] Catherine J. Cesarsky,et al. The Atacama Pathfinder EXperiment (APEX) : a new submillimeter facility for southern skies , 2006 .
[43] E. Pellegrini,et al. A Magnetically Supported Photodissociation Region in M17 , 2006, astro-ph/0611808.
[44] C. Wilson,et al. High-Mass Star Formation. II. The Mass Function of Submillimeter Clumps in M17 , 2006, astro-ph/0603330.
[45] R. Meijerink,et al. Diagnostics of irradiated dense gas in galaxy nuclei. II. A grid of XDR and PDR models , 2006, astro-ph/0610360.
[46] C. Kramer,et al. The cooling of atomic and molecular gas in DR21 , 2006, astro-ph/0609559.
[47] J. Black,et al. A computer program for fast non-LTE analysis of interstellar line spectra With diagnostic plots to interpret observed line intensity ratios , 2007, 0704.0155.
[48] H. Yamamoto,et al. Clumpy photon-dominated regions in Carina - I. [C I] and mid-J CO lines in two 4'$\times$4' fields , 2007, 0711.1320.
[49] R. Indebetouw,et al. THE EXTENDED ENVIRONMENT OF M17: A STAR FORMATION HISTORY , 2009, 0902.3280.