NAME Orion Peak 1 , the SIMBAD biblio

NAME Orion Peak 1 , the SIMBAD biblio (36 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.18CEST11:23:45


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Title First 3 Authors
1978ApJ...223..464B 6 9 282 Observations of the molecular hydrogen emission from the Orion nebula. BECKWITH S., PERSSON S.E., NEUGEBAUER G., et al.
1983ApJ...264..152B 1 9 80 Observations of the extinction and excitation of the molecular hydrogen emission in Orion. BECKWITH S., EVANS II N.J., GATLEY I., et al.
1989MNRAS.237.1009B 2 4 40 The velocity profile of the 1-0S(1) line of molecular hydrogen at Peak 1 in Orion. BRAND P.W.J.L., TONER M.P., GEBALLE T.R., et al.
1994ApJ...420..746S 58 19 Fabry-Perot imaging of molecular hydrogen emission in Orion-KL region. SUGAI H., USUDA T., KATAZA H., et al.
1995AJ....110.1295E 72 T                   4 17 Near-infrared spectroscopy towards the H2
peak in Orion.
EVERETT M.E., DEPOY D.L. and POGGE R.W.
1998AGAb...14...46R 71 T                   1 0 Shocked molecular hydrogen in Orion Pk1. ROSENTHAL D., BERTOLDI F., DRAPATZ S., et al.
1999A&A...346..267B 38   K                 6 48 Detection of HD in the Orion molecular outflow. BERTOLDI F., TIMMERMANN R., ROSENTHAL D., et al.
1999ApJ...520..162J 22 34 Low-velocity ionized winds from regions around young O stars. JAFFE D.T. and MARTIN-PINTADO J.
2000A&A...356..705R 3 11 130 ISO-SWS observations of OMC-1: H2 and fine structure lines. ROSENTHAL D., BERTOLDI F. and DRAPATZ S.
2000ApJ...530L.123S 1 5 15 Extended far-infrared CO emission in the OMC-1 core of Orion. SEMPERE M.J., CERNICHARO J., LEFLOCH B., et al.
2002A&A...386.1074G 74 T                   5 30 CO and H2O vibrational emission toward
Orion Peak 1 and Peak 2.
GONZALEZ-ALFONSO E., WRIGHT C.M., CERNICHARO J., et al.
2002A&A...389..374R 1 31 122 An ISO-SWS survey of molecular hydrogen in starburst and Seyfert galaxies. RIGOPOULOU D., KUNZE D., LUTZ D., et al.
2002A&A...390.1089P 2 63 485 The rich 6 to 9 µm spectrum of interstellar PAHs. PEETERS E., HONY S., VAN KERCKHOVEN C., et al.
2003A&A...399.1047B 36   K                 6 15 Gas-phase CO2, C2H2, and HCN toward Orion-KL. BOONMAN A.M.S., VAN DISHOECK E.F., LAHUIS F., et al.
2003A&A...411..427H 60 4 The stellar environment of SMC N81. HEYDARI-MALAYERI M., MEYNADIER F., CHARMANDARIS V., et al.
2004ApJ...611..928V 1 53 213 The profiles of the 3-12 micron polycyclic aromatic hydrocarbon features. VAN DIEDENHOVEN B., PEETERS E., VAN KERCKHOVEN C., et al.
2007A&A...466..949N viz 59 22 Observations of spatial and velocity structure in the Orion molecular cloud. NISSEN H.D., GUSTAFSSON M., LEMAIRE J.L., et al.
2007A&A...475L..15S 39           X         1 3 24 Low energy H+CO scattering revisited CO rotational excitation with new potential surfaces. SHEPLER B.C., YANG B.H., DHILIP KUMAR T.J., et al.
2011ApJ...737...96G 1214     A D     X C       32 24 81 Herschel measurements of molecular oxygen in Orion. GOLDSMITH P.F., LISEAU R., BELL T.A., et al.
2012ApJ...744...62N 76           X         2 7 7 Rovibrational quenching rate coefficients of HD in collisions with He. NOLTE J.L., STANCIL P.C., LEE T.-G., et al.
2013ApJ...771...49Y 38           X         1 20 17 Quantum calculation of inelastic CO collisions with H. I. Rotational quenching of low-lying rotational levels. YANG B., STANCIL P.C., BALAKRISHNAN N., et al.
2014ApJ...793..111C 2399     A D     X C       62 16 17 Herschel HIFI observations of O2 toward Orion: special conditions for shock enhanced emission. CHEN J.-H., GOLDSMITH P.F., VITI S., et al.
2015ApJ...799..102G 468       S   X C       10 21 32 Herschel far-infrared spectral-mapping of Orion BN/KL outflows: spatial distribution of excited CO, H2O, OH, O, and c+ in shocked gas. GOICOECHEA J.R., CHAVARRIA L., CERNICHARO J., et al.
2015ApJ...806..227M 1427     A     X C       36 10 13 O2 emission toward Orion H2
Peak 1 and the role of FUV-illuminated C-shocks.
MELNICK G.J. and KAUFMAN M.J.
2015A&A...581A..71F viz 1342       D     X C       34 20 23 Resolving the chemical substructure of Orion-KL. FENG S., BEUTHER H., HENNING T., et al.
2016ApJ...817..148O 39           X         1 18 5 IGRINS Near-IR high-resolution spectroscopy of multiple jets around LkHα 234. OH H., PYO T.-S., YUK I.-S., et al.
2016MNRAS.457.1593W 173       D       C F     3 67 5 Absorption at 11 mm in the interstellar medium and embedded sources: evidence for crystalline silicates. WRIGHT C.M., DO DUY T. and LAWSON W.
2016ApJ...833..275O 574   K A     X C       14 14 5 Three-dimensional shock structure of the Orion KL outflow with IGRINS. OH H., PYO T.-S., KAPLAN K., et al.
2018MNRAS.473.1472T 401           X C F     8 10 6 H2 emission from non-stationary magnetized bow shocks. TRAM L.N., LESAFFRE P., CABRIT S., et al.
2019A&A...622A..91G viz 82           X         2 17 23 Molecular tracers of radiative feedback in Orion (OMC-1). Widespread CH+ (J = 1-0), CO (10-9), HCN (6-5), and HCO+ (6-5) emission. GOICOECHEA J.R., SANTA-MARIA M.G., BRON E., et al.
2020A&A...636A.114F 27 ~ Deep search for hydrogen peroxide toward pre- and protostellar objects. Testing the pathway of grain surface water formation. FUCHS G.W., WITSCH D., HERBERTH D., et al.
2021A&A...648A..24V 43           X         1 64 73 Water in star-forming regions: physics and chemistry from clouds to disks as probed by Herschel spectroscopy. VAN DISHOECK E.F., KRISTENSEN L.E., MOTTRAM J.C., et al.
2021ApJ...916...52T 59       D     X         2 18 ~ The 3.3 µm infrared emission feature: observational and laboratory constraints on its carrier. TOKUNAGA A.T. and BERNSTEIN L.S.
2024ApJS..273...32L 45           X         1 9 ~ On the Interpretation of Mid-infrared Absorption Lines of Gas-phase H2O as Observed by JWST/MIRI. LI J., BOOGERT A. and TIELENS A.G.G.M.
2024RAA....24i5007W viz 18       D               3 42 ~ Molecular Oxygen Abundance in Galactic Massive Star Formation Regions Based on SWAS Observations. WANG B.-R., LI D., GOLDSMITH P.F., et al.
2025A&A...697A.186K 112       D     X         3 8 ~ SOFIA FIFI-LS spectroscopy of DR21 Main: Energetics of the spatially resolved outflow from a high-mass protostar. KARSKA A., FIGUEIRA M., MIROCHA A., et al.

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