The Mid-infrared Molecular Inventory toward Orion IRc2
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Timothy J. Lee | E. Herbst | C. DeWitt | N. Rangwala | S. Colgan | Xinchuan Huang | M. Drozdovskaya | R. Fortenberry | K. Acharyya | S. Nickerson | J. Monzon
[1] C. DeWitt,et al. Infrared H2O Absorption in Massive Protostars at High Spectral Resolution: Full Spectral Survey Results of AFGL 2591 and AFGL 2136 , 2022, The Astrophysical Journal.
[2] M. Juvela,et al. ATOMS: ALMA Three-millimeter Observations of Massive Star-forming regions -- VIII. A search for hot cores by using C$_2$H$_5$CN, CH$_3$OCHO and CH$_3$OH lines , 2022, 2201.10044.
[3] A. Ginsburg,et al. Structure of the Source I Disk in Orion-KL , 2021, The Astrophysical Journal.
[4] C. I. O. Technology.,et al. Mapping Physical Parameters in Orion KL at High Spatial Resolution , 2021, The Astrophysical Journal.
[5] S. Bovino,et al. On the low ortho-to-para H2 ratio in star-forming filaments , 2021, Astronomy & Astrophysics.
[6] N. Woolf,et al. Carbon Isotope Ratios in Planetary Nebulae: The Unexpected Enhancement of 13C , 2020, The Astrophysical Journal.
[7] Timothy J. Lee,et al. The First Mid-infrared Detection of HNC in the Interstellar Medium: Probing the Extreme Environment toward the Orion Hot Core , 2020, 2008.12787.
[8] D. Neufeld,et al. High-resolution Infrared Spectroscopy of Hot Molecular Gas in AFGL 2591 and AFGL 2136: Accretion in the Inner Regions of Disks around Massive Young Stellar Objects , 2020, The Astrophysical Journal.
[9] P. Caselli,et al. Carbon isotopic fractionation in molecular clouds , 2020, Astronomy & Astrophysics.
[10] A. Tielens,et al. The H2O Spectrum of the Massive Protostar AFGL 2136 IRS 1 from 2 to 13 μm at High Resolution: Probing the Circumstellar Disk , 2020, The Astrophysical Journal.
[11] J. He,et al. An experimental study of the surface formation of methane in interstellar molecular clouds , 2020, Nature Astronomy.
[12] G. Ferland,et al. Deciphering the 3D Orion Nebula-I: Expanding Shells in the Huygens Region , 2020, The Astrophysical Journal.
[13] A. Ginsburg,et al. Observations of the Orion Source I Disk and Outflow Interface , 2019, The Astrophysical Journal.
[14] Di Li,et al. Sulfur-bearing Molecules in Orion KL , 2019, The Astrophysical Journal.
[15] Johannes L. Schönberger,et al. SciPy 1.0: fundamental algorithms for scientific computing in Python , 2019, Nature Methods.
[16] E. Herbst,et al. Modeling C-shock Chemistry in Isolated Molecular Outflows , 2019, The Astrophysical Journal.
[17] V. Rivilla,et al. ALMA Observations of Ethyl Formate toward Orion KL , 2018, The Astrophysical Journal.
[18] A. Tielens,et al. High-resolution SOFIA/EXES Spectroscopy of SO2 Gas in the Massive Young Stellar Object MonR2 IRS3: Implications for the Sulfur Budget , 2018, The astrophysical journal. Letters.
[19] D. Neufeld,et al. Infrared Detection of Abundant CS in the Hot Core AFGL 2591 at High Spectral Resolution with SOFIA/EXES , 2018, The Astrophysical Journal.
[20] Jonathan C. Tan,et al. High Spectral Resolution Observations toward Orion BN at 6 μm: No Evidence for Hot Water , 2018, The Astrophysical Journal.
[21] E. Dishoeck,et al. The ALMA-PILS survey: isotopic composition of oxygen-containing complex organic molecules toward IRAS 16293–2422B , 2018, Astronomy & Astrophysics.
[22] E. Herbst,et al. Hot Cores in Magellanic Clouds , 2018 .
[23] F. Lique,et al. Abundance of HCN and its C and N isotopologues in L1498 , 2018, Astronomy & Astrophysics.
[24] Miguel de Val-Borro,et al. The Astropy Project: Building an Open-science Project and Status of the v2.0 Core Package , 2018, The Astronomical Journal.
[25] V. Wakelam,et al. A new look at sulphur chemistry in hot cores and corinos , 2017, 1711.11406.
[26] G. Nyman,et al. H$_2$ formation on interstellar dust grains: the viewpoints of theory, experiments, models and observations , 2017, 1711.10568.
[27] Eric Herbst,et al. High Spectral Resolution SOFIA/EXES Observations of C2H2 toward Orion IRc2 , 2017, 1709.04084.
[28] S. Qin,et al. ALMA Observations of the Archetypal “Hot Core” That Is Not: Orion-KL , 2017, 1708.08448.
[29] L. Looney,et al. CARMA λ = 1 cm Spectral Line Survey of Orion-KL , 2017, 1708.06776.
[30] M. Honma,et al. Disk-driven rotating bipolar outflow in Orion Source I , 2017, Nature Astronomy.
[31] J. Rizzo,et al. A spectroscopic survey of Orion KL between 41.5 and 50 GHz. , 2017, Astronomy and astrophysics.
[32] M. Wright,et al. ALMA Images of the Orion Hot Core at 349 GHz , 2017, 1705.03957.
[33] G. Ferland,et al. Which Stars Are Ionizing the Orion Nebula? , 2017, 1703.06191.
[34] A. Ginsburg,et al. The ALMA View of the OMC1 Explosion in Orion , 2017, 1701.01906.
[35] Jonathan Tennyson,et al. The 2015 edition of the GEISA spectroscopic database , 2016 .
[36] Laurence S. Rothman,et al. HITRAN Application Programming Interface (HAPI): A comprehensive approach to working with spectroscopic data , 2016 .
[37] B. Jiang,et al. A PRECISE DETERMINATION OF THE MID-INFRARED INTERSTELLAR EXTINCTION LAW BASED ON THE APOGEE SPECTROSCOPIC SURVEY , 2016, 1602.02928.
[38] K. Menten,et al. A 1.3 cm Line Survey toward Orion KL , 2015, 1506.03235.
[39] S. Viti,et al. A new study of an old sink of sulphur in hot molecular cores: the sulphur residue , 2015, 1503.07227.
[40] Devin W. Silvia,et al. The Orion Fingers: Near-IR Adaptive Optics Imaging of an Explosive Protostellar Outflow , 2015, 1502.04711.
[41] G. Bilalbegović,et al. Sulfur-bearing species in molecular clouds , 2014, 1410.8293.
[42] E. Bergin,et al. 13C–METHYL FORMATE: OBSERVATIONS OF A SAMPLE OF HIGH-MASS STAR-FORMING REGIONS INCLUDING ORION–KL AND SPECTROSCOPIC CHARACTERIZATION , 2014, 1410.4418.
[43] P. Caselli,et al. Chemistry and radiative transfer of water in cold, dense clouds , 2014, 1403.0155.
[44] Jonathan Tennyson,et al. ExoMol line lists - III. An improved hot rotation-vibration line list for HCN and HNC , 2013, 1311.1328.
[45] M. Gerin,et al. Nitrogen isotopic ratios in Barnard 1: a consistent study of the N2H+, NH3, CN, HCN, and HNC isotopologues , 2013, 1309.5782.
[46] Prasanth H. Nair,et al. Astropy: A community Python package for astronomy , 2013, 1307.6212.
[47] T. Henning,et al. Resolving the chemical substructure of Orion-KL , 2013, 1504.08012.
[48] L. Pagani,et al. Ortho-H2 and the age of prestellar cores , 2013 .
[49] A. Bolatto,et al. The CO-to-H2 Conversion Factor , 2013, 1301.3498.
[50] H. Rix,et al. MOLECULAR GAS AND STAR FORMATION IN NEARBY DISK GALAXIES , 2013, 1301.2328.
[51] J. Bally,et al. A 3D view of the outflow in the Orion Molecular Cloud 1 (OMC-1) , 2012, 1203.3056.
[52] Daniel Foreman-Mackey,et al. emcee: The MCMC Hammer , 2012, 1202.3665.
[53] J. Tennyson,et al. ExoMol: molecular line lists for exoplanet and other atmospheres , 2012, 1204.0124.
[54] H. Kataza,et al. Physical Relation of Source I to IRc2 in the Orion KL Region , 2011, 1104.4394.
[55] D. Despois,et al. HCOOCH3 as a probe of temperature and structure in Orion-KL , 2011, 1103.2548.
[56] Luis A. Zapata Johannes Schmid-Burgk Karl M. Menten. Orion KL: the hot core that is not a , 2010, 1009.1426.
[57] J. Goicoechea,et al. A line-confusion limited millimeter survey of Orion KL - II. Silicon-bearing species , 2010, 1012.1969.
[58] F. Adams. The Birth Environment of the Solar System , 2010, 1001.5444.
[59] T. Henning,et al. Disk and outflow signatures in Orion-KL: the power of high-resolution thermal infrared spectroscopy , 2010, 1001.0650.
[60] C. Ceccarelli,et al. Constraining the ortho-to-para ratio of H2 with anomalous H2CO absorption , 2009 .
[61] G. Ferland,et al. Spitzer reveals what's behind Orion's Bar , 2009, Proceedings of the International Astronomical Union.
[62] S. Bontemps,et al. S-bearing molecules in massive dense cores , 2009, 0906.1122.
[63] S. Sakai,et al. SiO Maser Observations toward Orion-KL with VERA , 2008 .
[64] P. Bernath,et al. A spectral line survey of Orion KL in the bands 486-492 and 541-577 GHz with the Odin satellite II. Data analysis , 2007, 0910.1815.
[65] P. Bernath,et al. A spectral line survey of Orion KL in the bands 486-492 and 541-577 GHz with the Odin satellite: I. The observational data , 2007, 0910.1825.
[66] R. Garrod,et al. Molecular Evolution and Star Formation: From Prestellar Cores to Protostellar Cores , 2007, 0710.0712.
[67] Urbana,et al. Kinematics and Chemistry of the Hot Molecular Core in G34.26+0.15 at High Resolution , 2007, astro-ph/0701827.
[68] M. Barlow,et al. A far-infrared molecular and atomic line survey of the Orion KL region , 2006, astro-ph/0605410.
[69] University of Wales,et al. Hubble Space Telescope NICMOS Polarization Measurements of OMC-1 , 2006, astro-ph/0601077.
[70] J. Tennyson,et al. Improved HCN/HNC linelist, model atmospheres and synthetic spectra for WZ Cas , 2005, astro-ph/0512363.
[71] Gang Li,et al. The HITRAN 2008 molecular spectroscopic database , 2005 .
[72] M. A. Brewster,et al. The 12C/13C Isotope Gradient Derived from Millimeter Transitions of CN: The Case for Galactic Chemical Evolution , 2005 .
[73] D. Rouan,et al. Observations of spatial and velocity structure in the Orion molecular cloud , 2005, astro-ph/0511226.
[74] L. Loinard,et al. Dynamical Decay of a Massive Multiple System in Orion KL? , 2005, astro-ph/0509201.
[75] B. Draine,et al. H2 Pure Rotational Lines in the Orion Bar , 2005, astro-ph/0506003.
[76] F. Motte,et al. A Molecular Line Survey of Orion KL in the 350 Micron Band , 2005 .
[77] G. Blake,et al. Methane Abundance Variations toward the Massive Protostar NGC 7538 IRS 9 , 2004, astro-ph/0407270.
[78] P. Caselli,et al. Resetting chemical clocks of hot cores based on S-bearing molecules , 2004, astro-ph/0404246.
[79] P. Tuthill,et al. High Angular Resolution Mid-Infrared Imaging of Young Stars in Orion BN/KL , 2004, astro-ph/0402423.
[80] J. Bally,et al. A New Mid-Infrared Map of the BN/KL Region Using the Keck Telescope , 2003, astro-ph/0404115.
[81] E. F. Dishoeck,et al. Gas-phase CO2, C2H2, and HCN toward Orion-KL , 2003 .
[82] F. D. Tak,et al. Sulphur chemistry in the envelopes of massive young stars , 2002, astro-ph/0212325.
[83] R. Neri,et al. On the Heating Source of the Orion KL Hot Core , 2002, astro-ph/0206504.
[84] J. Takahashi. The Ortho/Para Ratio of H2 Newly Formed on Dust Grains , 2001 .
[85] D. Jaffe,et al. TEXES: A Sensitive High‐Resolution Grating Spectrograph for the Mid‐Infrared , 2001, astro-ph/0110521.
[86] E. F. Dishoeck,et al. Gas-phase SO2 in absorption towards massive protostars , 2001 .
[87] D. Lis,et al. A Line Survey of Orion-KL from 607 to 725 GHz , 2001 .
[88] K. Johnston,et al. Kinematics, Kinetic Temperatures, and Column Densities of NH3 in the Orion Hot Core , 2000 .
[89] T. Millar,et al. On the Abundance Gradients of Organic Molecules along the TMC-1 Ridge , 2000 .
[90] W. Irvine,et al. The Formaldehyde Ortho/Para Ratio as a Probe of Dark Cloud Chemistry and Evolution , 1999, The Astrophysical journal.
[91] P. Goldsmith,et al. Population Diagram Analysis of Molecular Line Emission , 1999 .
[92] C. Gwinn,et al. Coexisting conical bipolar and equatorial outflows from a high-mass protostar , 1998, Nature.
[93] Bart Vandenbussche,et al. The ISO-SWS 2.4-45.2 Micron Spectrum toward Orion IRc2 , 1998 .
[94] A. Tielens,et al. High-Temperature Molecular Cores near Massive Stars and Application to the Orion Hot Core , 1998 .
[95] M. P. Gutiérrez,et al. Shock Chemistry in the Young Bipolar Outflow L1157 , 1997 .
[96] S. Charnley. Sulfuretted Molecules in Hot Cores , 1997 .
[97] L. Mundy,et al. A λ = 1.3 Millimeter Aperture Synthesis Molecular Line Survey of Orion Kleinmann-Low , 1996 .
[98] M. Wright,et al. A Multiline Aperture Synthesis Study of Orion-KL , 1996 .
[99] K. Menten,et al. What is Powering the Orion Kleinmann-Low Infrared Nebula? , 1995 .
[100] N. Evans,et al. Observation of infrared and radio lines of molecules toward GL 2591 and comparison to physical and chemical models , 1995, astro-ph/9505115.
[101] W. Danchi,et al. The distribution of molecules in the core of OMC-1 , 1995 .
[102] J. Lacy,et al. Shocked pure-rotational emission from H2 in Orion , 1994 .
[103] È. Roueff,et al. Sulphur-bearing molecules as tracers of shocks in interstellar clouds , 1993 .
[104] S. Lord. A new software tool for computing Earth's atmospheric transmission of near- and far-infrared radiation , 1992 .
[105] D. Gezari. Mid-infrared imaging of Orion BN/KL : astrometry of IRc2 and the SiO maser , 1992 .
[106] E. Herbst,et al. Models of gas-grain chemistry in dense interstellar clouds with complex organic molecules , 1992 .
[107] N. Evans,et al. Infrared Molecular Spectroscopy toward the Orion IRc2 and IRc7 Sources: A New Probe of Physical Conditions and Abundances in Molecular Clouds , 1991 .
[108] Neal J. Evans,et al. Discovery of interstellar methane - Observations of gaseous and solid CH4 absorption toward young stars in molecular clouds , 1991 .
[109] M. Allen,et al. Hot and cold gas toward young stellar objects , 1990 .
[110] Y. Murata,et al. APERTURE SYNTHESIS OBSERVATIONS OF NH-3 IN OMC-1: FILAMENTARY STRUCTURES AROUND ORION-KL , 1990 .
[111] N. Evans,et al. Discovery of interstellar acetylene , 1989 .
[112] T. Geballe,et al. The velocity profile of the 1 – 0 S(1) line of molecular hydrogen at Peak 1 in Orion , 1989 .
[113] J. Stutzki,et al. The Orion Molecular Cloud and Star-Forming Region , 1988 .
[114] S. E. Persson,et al. Images of star-forming regions. III. Sources in the NGC 7538 molecular cloud complex , 1988 .
[115] M. Felli,et al. Solar system-sized condensations in the Orion Nebula , 1987 .
[116] Geoffrey A. Blake,et al. Molecular abundances in OMC-1 - the chemical composition of interstellar molecular clouds and the influence of massive star formation , 1987 .
[117] E. Becklin,et al. The Kleinmann-Low nebula - An infrared cavity , 1984 .
[118] S. Beck. The structure of high-velocity gas in Orion and the possible role of IRc9 , 1984 .
[119] S. Ridgway,et al. The circumstellar and nebular environment of the Becklin-Neugebauer object - 2-5 micron wavelength spectroscopy , 1983 .
[120] R. Genzel,et al. NH3 in Orion-KL - A new interpretation , 1982 .
[121] M. Oppenheimer,et al. Molecular diagnostics of interstellar shocks , 1980 .
[122] A. H. Barrett,et al. Ammonia observations of the Orion molecular cloud. , 1979 .
[123] F. Gillett,et al. Infrared observations of the OH source W33 A , 1978 .
[124] S. E. Persson,et al. Observations of the molecular hydrogen emission from the Orion Nebula , 1978 .
[125] G. Rieke,et al. High-Resolution Maps of the Kleinmann-Low Nebula in Orion , 1973 .
[126] Frank J. Low,et al. Discovery of an infrared nebula in Orion. , 1967 .
[127] G. Neugebauer,et al. Observations of an infrared star in the Orion nebula. , 1967 .
[128] E. Murphy,et al. Science with a next-generation Very Large Array , 2019 .
[129] N. Evans,et al. The c2d Spitzer Spectroscopic Survey of Ices around Low-Mass Young Stellar Objects. III. CH4 , 2008 .
[130] E. F. Dishoeck,et al. Chemical evolution of star-forming regions. , 1998, Annual review of astronomy and astrophysics.
[131] T G Phillips,et al. A Line Survey of Orion KL from 325 to 360 GHz , 1997, The Astrophysical journal. Supplement series.