NAME Serpens SVS 4 IR Cluster , the SIMBAD biblio

NAME Serpens SVS 4 IR Cluster , the SIMBAD biblio (38 results) C.D.S. - SIMBAD4 rel 1.7 - 2020.10.20CEST09:06:15

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Title First 3 Authors
2012A&A...538A..91D 46           X         1 5 30 Production of interstellar hydrogen peroxide (H2O2) on the surface of dust grains. DU F., PARISE B. and BERGMAN P.
2012ApJS..201...11K viz 257       D     X   F     6 105 20 Mid-infrared spectral variability atlas of young stellar objects. KOSPAL A., ABRAHAM P., ACOSTA-PULIDO J.A., et al.
2011ApJ...742...28W 135 36 Observational constraints on methanol production in interstellar and preplanetary ices. WHITTET D.C.B., COOK A.M., HERBST E., et al.
2010ApJ...716..299S 315           X C       7 49 27 Near-infrared imaging polarimetry of the Serpens cloud core: magnetic field structure, outflows, and inflows in a cluster forming clump. SUGITANI K., NAKAMURA F., TAMURA M., et al.
2010ApJ...716..634G 236           X C       5 92 10 FLAMINGOS near infrared survey of the Serpens cloud main core. GORLOVA N., STEINHAUER A. and LADA E.
2010ApJ...718..610D 555       S   X         13 14 120 VLBA determination of the distance to nearby star-forming regions. IV. A preliminary distance to the Proto-Herbig AeBe star EC 95 in the Serpens core. DZIB S., LOINARD L., MIODUSZEWSKI A.J., et al.
2009A&A...494L..13O 250       D     X         7 12 20 Cold gas as an ice diagnostic toward low mass protostars. OEBERG K.I., BOTTINELLI S. and VAN DISHOECK E.F.
2008ApJ...685.1033P 15       D               2 18 22 Detection of C3 O in the low-mass protostar Elias 18. PALUMBO M.E., LETO P., SIRINGO C., et al.
2005AJ....130..643E 29 21 Very large array 3.5 cm continuum sources in the Serpens cloud core. EIROA C., TORRELLES J.M., CURIEL S., et al.
2004A&A...421..623K viz 167 67 The young stellar population in the Serpens Cloud Core: An ISOCAM survey. KAAS A.A., OLOFSSON G., BONTEMPS S., et al.
2004A&A...423..241S 2 8 33 Models of gas-grain chemistry in interstellar cloud cores with a stochastic approach to surface chemistry. STANTCHEVA T. and HERBST E.
2004A&A...426..925P 2 17 86 Mapping ices in protostellar environments on 1000 AU scales. Methanol-rich ice in the envelope of Serpens SMM 4. PONTOPPIDAN K.M., VAN DISHOECK E.F. and DARTOIS E.
2004ApJS..150..343E viz 254 8 A uniform database of 2.2-16.5 µm spectra from the ISOCAM CVF spectrometer. ENGELKE C.W., KRAEMER K.E. and PRICE S.D.
2004ApJS..151..299H viz 922 16 Classification of spectra from the infrared space observatory PHT-s database. HODGE T.M., KRAEMER K.E., PRICE S.D., et al.
2003A&A...397..177B viz 284 88 A Catalogue of infrared star clusters and stellar groups. BICA E., DUTRA C.M. and BARBUY B.
2003A&A...401..613A viz         O           61 36 ISOCAM-CVF spectroscopy of the circumstellar environment of young stellar objects. ALEXANDER R.D., CASALI M.M., ANDRE P., et al.
2003A&A...404L..17P 4         O           9 72 Detection of abundant solid methanol toward young low mass stars. PONTOPPIDAN K.M., DARTOIS E., VAN DISHOECK E.F., et al.
2003AJ....126.1916P viz 92 89 A catalog of young stellar groups and clusters within 1 kiloparsec of the Sun. PORRAS A., CHRISTOPHER M., ALLEN L., et al.
2003Msngr.113...49V 21 11 Origin and evolution of ices in star-forming regions - a VLT-ISAAC 3-5 mum spectroscopic survey. VAN DISHOECK E., DARTOIS E., PONTOPPIDAN K.M., et al.
2000A&A...363..253L 23 28 The ISO-LWS map of the Serpens cloud core. I. The SEDs of the IR/SMM sources. LARSSON B., LISEAU R., MEN'SHCHIKOV A.B., et al.
1999A&A...345..583P 13 21 An extremely X-ray luminous proto-Herbig Ae/Be star in the Serpens star forming region. PREIBISCH T.
1998A&A...338L..25P 16 22 Super-strong X-ray emission from a deeply embedded young stellar object in the Serpens cloud core. PREIBISCH T.
1998ApJ...498..716C 1 23 85 Processing of icy mantles in protostellar envelopes. CHIAR J.E., GERAKINES P.A., WHITTET D.C.B., et al.
1997ApJ...479..818E 1 17 68 The 2140 cm–1 (4.673 micron) solid CO band: the case for interstellar O2 and N2 and the photochemistry of nonpolar interstellar ice analogs. ELSILA J., ALLAMANDOLA L.J. and SANDFORD S.A.
1996A&A...315L.189G 20 44 Detection of an absorption feature at the position of the 4.27-µm band of solid CO2. GUERTLER J., HENNING T., KOEMPE C., et al.
1996ApJ...460L..45H 2 13 84 A cluster of class 0 protostars in Serpens: an IRAS HIRES study. HURT R.L. and BARSONY M.
1995ApJ...441..222B 4 13 166 Gas-phase chemistry in dense interstellar clouds including grain surface molecular depletion and desorption. BERGIN E.A., LANGER W.D. and GOLDSMITH P.F.
1995ApJ...455..234C 1 46 159 High-resolution studies of solid CO in the Taurus Dark Cloud: characterizing the ices in quiescent clouds. CHIAR J.E., ADAMSON A.J., KERR T.H., et al.
1995MmSAI..66..685K 4 2 How to identify embedded young stellar objects : a case study of the Serpens Cloud Core. KAAS A.A., OLOFSSON G. and FRIDLUND M.
1994ApJ...426..240C 2 9 74 Solid carbon monoxide in the Serpens dark cloud. CHIAR J.E., ADAMSON A.J., KERR T.H., et al.
1992A&A...262..468E 163 108 Near-infrared images of the Serpens cloud core: the stellar cluster. EIROA C. and CASALI M.M.
1992PASJ...44..155E 72 T                   3 9 Molecular outflows in the Serpens cloud core ?: FIRS 1 and SVS 4. EIROA C., TORRELLES J.M., GOMEZ J.F., et al.
1989A&A...210..345E 1 9 69 Ice dust grains in the Serpens molecular cloud. EIROA C. and HODAPP K.-W.
1989A&A...223L..17E 71 T                   1 14 39 The Serpens sources
SVS 4 and FIRS 1 : new results from infrared images.
1989ApL....27..299C 25 ~ Extended radio continuum emission associated with V645 Cyg and MWC 1080. CURIEL S., RODRIGUEZ L.F., CANTO J., et al.
1988A&A...196..236Z 1 7 28 IRAS study of the Serpens molecular cloud. II. The Serpens core. ZHANG C.Y., LAUREIJS R.J. and CLARK F.O.
1988A&A...201..299G 20 38 Observational evidence for the influence of the magnetic field on star formation in the Serpens molecular cloud. GOMEZ DE CASTRO A.I., EIROA C. and LENZEN R.
1976AJ.....81..638S 40 86 Infrared surveys of dark cloud complexes. V. The NGC 7129 region and the Serpens dark cloud. STROM S.E., VRBA F.J. and STROM K.M.

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