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The Astrophysical Journal Supplement Series, ISSN 0067-0049, 10/2005, Volume 160, Issue 2, pp. 319 - 352
Journal Article
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 6/2002, Volume 332, Issue 4, pp. 985 - 993
Abstract We report calculations of the intensities of rovibrational transitions of H2 emitted from C-type shock waves propagating in molecular gas. Attention... 
molecular processes | ISM: molecules | ISM: individual: Orion OMC‐1 | shock waves | ISM: individual: orion OMC-1 | Shock waves | Molecular processes | ATOMIC-HYDROGEN | ISM : individual : Orion OMC-1 | RATIO | ISM : molecules | H-2 | COLLISIONAL EXCITATION | LINES | TRANSITION | GRAINS | OMC-1 | ASTRONOMY & ASTROPHYSICS | EMISSION | MAGNETOHYDRODYNAMIC SHOCKS
Journal Article
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 2017, Volume 472, Issue 1, pp. 738 - 743
Among interstellar chlorine bearing molecules, HCl is certainly the most useful probe for studying chlorine chemistry since it is formed at the end of the... 
Molecular processes | Molecular data | ISM: abundances | RATE COEFFICIENTS | CROSS-SECTIONS | HYDROGEN-CHLORIDE | molecular data | OMC-1 | ASTRONOMY & ASTROPHYSICS | molecular processes | INTERSTELLAR-MEDIUM | ABUNDANCE | Physics
Journal Article
by Li, MY and Zhou, JJ and Esimbek, J and Quan, DH and He, YX and Li, Q and Zhu, CH
ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES, ISSN 0067-0049, 07/2019, Volume 243, Issue 1, p. 13
We selected 90 massive star-forming clumps with strong N2H+(1-0), HCO+(1-0), HCN(1-0), and HNC(1-0) emission from the Millimetre Astronomy Legacy Team 90 GHz... 
stars: formation | HCN | radio lines: ISM | OMC-1 | ISM: molecules | ASTRONOMY & ASTROPHYSICS | ISM: kinematics and dynamics | RATIO | HCO+ EMISSION | HNC | REGION | Temperature rise | Temperature | Emission | Abundance | Sky surveys (astronomy) | Density | Pixels | Emissions | Massive stars | Surveys | Organic chemistry | Star formation | Continuum radiation | Clumps | Chemical properties | Astronomy | Physics - Astrophysics of Galaxies
Journal Article
The Astrophysical Journal, ISSN 0004-637X, 11/2011, Volume 741, Issue 2, pp. 112 - jQuery1323901896380='48'
Journal Article
Journal Article
Astrophysical Journal, ISSN 0004-637X, 02/2017, Volume 836, Issue 1, p. 117
Journal Article
Journal of Chemical Physics, ISSN 0021-9606, 06/2015, Volume 142, Issue 24, p. 241102
Journal Article
The Astrophysical Journal Supplement Series, ISSN 0067-0049, 02/2005, Volume 156, Issue 2, pp. 127 - 167
With the Caltech Submillimeter Observatory, we have carried out an unbiased spectral line survey of Orion KL throughout the 350 mum band (from 795 to 903 GHz).... 
Line: formation | Line: identification | ISM: molecules | Ism: abundances | ISM: individual (Orion) | Submillimeter | CORE | APERTURE SYNTHESIS | ISM : abundances | ISM : molecules | line : formation | INTERSTELLAR CLOUDS | submillimeter | 1ST DETECTION | ISM : individual (Orion) | OMC-1 | ASTRONOMY & ASTROPHYSICS | GHZ | NEBULA | IRC2 | EMISSION | KLEINMANN-LOW | line : identification
Journal Article
Astronomy and astrophysics, ISSN 0004-6361, 12/2014, Volume 572, pp. L10 - 6
Context. The ortho-to-para ratio (OPR) of H2O is thought to be sensitive to the temperature of water formation. The OPR of H2O is thus useful for studying the... 
ISM: individual objects: Orion Bar | ISM: molecules | ISM: individual objects: Orion S | MOLECULAR CLOUDS | LINE OBSERVATIONS | HIFI | SUBMILLIMETER OBSERVATIONS | INTERSTELLAR-MEDIUM | REGION | VAPOR | BAR | OMC-1 | ASTRONOMY & ASTROPHYSICS | CHEMISTRY | Protoplanets | Mathematical analysis | Texts | Formations | Gas temperature | Estimates | Density | Astronomy | Physics - Astrophysics of Galaxies
Journal Article
Journal Article
Astrophysical Journal Letters, ISSN 2041-8205, 03/2017, Volume 838, Issue 1, pp. L3 - L3
Journal Article
The Astrophysical Journal, ISSN 0004-637X, 07/2010, Volume 717, Issue 2, pp. 1262 - 1273
Journal Article
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 09/2005, Volume 362, Issue 3, pp. 995 - 1005
ABSTRACT The Australia Telescope Compact Array (ATCA) has been used to search for methanol maser emission at 6.7 GHz towards the Orion Molecular Cloud 1... 
ISM: individual: OMC‐1 | ISM: molecules | masers | Masers | ISM: individual: OMC-1 | ISM : individual : OMC-1 | FREQUENCIES | CENTIMETER | ISM : molecules | STAR-FORMING REGIONS | ORION REGION | DUST | PROTOSTELLAR OUTFLOWS | ASTRONOMY & ASTROPHYSICS | GHZ | MOLECULAR CLOUD CORES | TRANSITIONS | EMISSION | Arrays | Methanol | Emissions
Journal Article