NAME rho Oph W , the SIMBAD biblio

NAME rho Oph W , the SIMBAD biblio (28 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.18CEST19:48:27

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Bibcode/DOI Score in Title|Abstract|
Keywords 		in a table in teXt, Caption, ... Nb occurence Nb objects in ref Citations
(from ADS) 		Title First 3 Authors
1996A&A...315L.329A 3 10 131 ISOCAM mapping of the ρ Ophiuchi main cloud. ABERGEL A., BERNARD J.P., BOULANGER F., et al.
2003A&A...397..623H 4 5 71 H2 infrared line emission across the bright side of the ρ Ophiuchi main cloud. HABART E., BOULANGER F., VERSTRAETE L., et al.
2004A&A...414..531H 5 8 142 Some empirical estimates of the H2 formation rate in photon-dominated regions. HABART E., BOULANGER F., VERSTRAETE L., et al.
2004A&A...417..135T 1 17 79 Carbon budget and carbon chemistry in Photon Dominated Regions. TEYSSIER D., FOSSE D., GERIN M., et al.
2004ARA&A..42..119V 87 222 ISO spectroscopy of gas and dust : from molecular clouds to protoplanetary disks. VAN DISHOECK E.F.
2004AAS...205.1502W 5 0 WIYN/Hydra observations of the surface population of the rho Oph cloud. WILKING B.A., MEYER M.R., ROBINSON J.G., et al.
2006MNRAS.365..801P 7 19 Molecular hydrogen formation on porous dust grains. PERETS H.B. and BIHAM O.
2008ApJS..175..277D viz 15       D               7164 308 The SCUBA legacy catalogues: submillimeter-continuum objects detected by SCUBA. DI FRANCESCO J., JOHNSTONE D., KIRK H., et al.
2008A&A...483..495C 37           X         1 8 9 The role of carbon grains in the deuteration of H2. CAZAUX S., CASELLI P., COBUT V., et al.
2008MNRAS.391.1075C 3502     A D     X C       94 22 61 Centimetre-wave continuum radiation from the ρ Ophiuchi molecular cloud. CASASSUS S., DICKINSON C., CLEARY K., et al.
2009ApJ...699..150S viz 37           X         1 295 80 The evolution of massive young stellar objects in the large Magellanic cloud. I. Identification and spectral classification. SEALE J.P., LOONEY L.W., CHU Y.-H., et al.
2009ApJ...704..274L 16       D               1 8 27 Molecular hydrogen formation catalyzed by polycyclic aromatic hydrocarbons in the interstellar medium. LE PAGE V., SNOW T.P. and BIERBAUM V.M.
2010ApJ...710.1247S viz 15       D               1 761 87 The mass distribution of starless and protostellar cores in Gould Belt clouds. SADAVOY S.I., DI FRANCESCO J., BONTEMPS S., et al.
2011MNRAS.411.1137C 38           X         1 25 20 Dust-correlated centimetre-wave radiation from the M78 reflection nebula. CASTELLANOS P., CASASSUS S., DICKINSON C., et al.
2011A&A...536A..20P 154           X         4 31 177 Planck early results. XX. New light on anomalous microwave emission from spinning dust grains. PLANCK COLLABORATION, ADE P.A.R., AGHANIM N., et al.
2012ApJ...752....3T 50           X         1 1 24 Experimental evidence for the formation of highly superhydrogenated polycyclic aromatic hydrocarbons through H atom addition and their catalytic role in H2Formation. THROWER J.D., JORGENSEN B., FRIIS E.E., et al.
2012A&A...542A..69P 284       D     X C       7 15 69 Evaporating very small grains as tracers of the UV radiation field in photo-dissociation regions. PILLERI P., MONTILLAUD J., BERNE O., et al.
2015A&A...579A..72B 42           X         1 3 20 H2 formation on PAHs in photodissociation regions: a high-temperature pathway to molecular hydrogen. BOSCHMAN L., CAZAUX S., SPAANS M., et al.
2017ApJ...843...92B 42           X         1 9 52 The H I-to-H2 transition in a turbulent medium. BIALY S., BURKHART B. and STERNBERG A.
2018MNRAS.480.3224J 42           X         1 7 17 The C-Band All-Sky Survey (C-BASS): design and capabilities. JONES M.E., TAYLOR A.C., AICH M., et al.
2020ApJ...892...69B 140       D S   X         3 18 ~ A two carrier families spectral profile model for anomalous microwave emission. BERNSTEIN L.S., SHROLL R.M., QUENNEVILLE J., et al.
2020MNRAS.495.3482A 1111     A D     X C       27 12 ~ Resolved observations at 31 GHz of spinning dust emissivity variations in ρ Oph. ARCE-TORD C., VIDAL M., CASASSUS S., et al.
2021MNRAS.502..589C 1697 T K A     X C       39 16 ~ Resolved spectral variations of the centimetre-wavelength continuum from the ρ Oph W photodissociation region. CASASSUS S., VIDAL M., ARCE-TORD C., et al.
2022A&A...663A..65Y 43           X         1 12 3 Spinning nano-carbon grains: Viable origin for anomalous microwave emission. YSARD N., MIVILLE-DESCHENES M.-A., VERSTRAETE L., et al.
2024A&A...685A..73H 45           X         1 64 ~ PDRs4All II. JWST's NIR and MIR imaging view of the Orion Nebula. HABART E., PEETERS E., BERNE O., et al.
2025A&A...695A.245G 47           X         1 25 ~ QUIJOTE scientific results XVIII. New constraints on the polarisation of the anomalous microwave emission in bright Galactic regions: ρ Ophiuchi, Perseus, and W43. GONZALEZ-GONZALEZ R., GENOVA-SANTOS R.T., RUBINO-MARTIN J.A., et al.
2026A&A...706A.135H 50           X         1 4 ~ Formation of methane and cyclohexane through the hydrogenation of toluene. HOPKINSON A.T., DOKTOR F.G., PITFIELD J., et al.
2026A&A...707A.255C 1430 T K A S   X C       26 11 ~ ALMA Band 1 observations of the ρ Oph W filament I. Enhanced power from excess microwave emission at high spatial frequencies. CASASSUS S., VIDAL M., CARCAMO M., et al.

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