NAME GGD 27 IRS , the SIMBAD biblio

NAME GGD 27 IRS , the SIMBAD biblio (26 results) C.D.S. - SIMBAD4 rel 1.8 - 2024.04.19CEST01:52:59

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Keywords 		in a table in teXt, Caption, ... Nb occurence Nb objects in ref Citations
(from ADS) 		Title First 3 Authors
1987A&A...177..258Y 71 T                   1 8 48 Polarimetric mapping of a new infrared reflection nebula
GGD 27 IRS. 		YAMASHITA T., SATO S., NAGATA T., et al.
1990ApJ...364..232B 64 121 Parameters of disks around young stellar objects from polarization observations. BASTIEN P. and MENARD F.
1990ApJ...365..615Y 70 T                   1 6 13 The density structure of the protostellar disk: a power-law distribution of the dust around
GGD 27 IRS. 		YAMASHITA T., SATO S., KAIFU N., et al.
1991A&A...252..299A 70 T                   20 29 Near-IR imaging and spectroscopy of
GGD 27-IRS. 		ASPIN C., McCAUGHREAN M.J., CASALI M.M., et al.
1991ApJ...373..560Y 70 T                   1 5 13 The dense, inner part of the protostellar disk: protostar candidates in
GGD 27 IRS. 		YAMASHITA T., MURATA Y., KAWABE R., et al.
1992A&A...266..219A 70 T                   14 30 Mid-IR spectroscopy of
GGD 27-IRS : evidence for a PMS stellar cluster. 		ASPIN C. and GEBALLE T.R.
1993BAAS...25.1367A 71 T                   1 ~ Optical, near-infrared and mid-infrared imaging of
GGD27-IRS. 		ASPIN C., BLANCO P. and PINA R.
1994A&A...281L..29A 71 T                   9 15 Scattered near-IR CO emission bands in
GGD 27-IRS. Observing the circumstellar environment of heavily obscured young PMS stars. 		ASPIN C.
1994A&A...292L...9A 106 T K                 5 17 Thermal infrared imaging of
GGD27-IRS. The active pre-main sequence star revealed. 		ASPIN C., PUXLEY P.J., BLANCO P.R., et al.
1994ApJ...435L.145G 19 44 Ammonia downstream from HH 80 North. GIRART J.M., RODRIGUEZ L.F., ANGLADA G., et al.
1997ApJ...479..339S 13 20 High-resolution infrared observations of GGD 27. STECKLUM B., FELDT M., RICHICHI A., et al.
1997ApJ...480..255G 14 25 Submillimeter polarimetry of class 0 protostars: constraints on magnetized outflow models. GREAVES J.S., HOLLAND W.S. and WARD-THOMPSON D.
1999PASJ...51..819S 25 8 A study of the molecular cloud toward the HII regions S 35 and S 37 with NANTEN. SAITO H., TACHIHARA K., ONISHI T., et al.
2000MNRAS.311..522A 81 30 Herbig-Haro flows near compact reflection nebulae. ASPIN C. and REIPURTH B.
2000AcApS..20..383W 67 2 Searches for massive molecular cloud cores with CO isotopes. WU Y.-F., WU J.-W., WANG J.-Z., et al.
2002A&A...387..977F 57 52 The history of mass dispersal around Herbig Ae/Be stars. FUENTE A., MARTIN-PINTADO J., BACHILLER R., 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.
2002MNRAS.330.1034P 62 15 ISO -LWS two-colour diagram of young stellar objects. PEZZUTO S., GRILLO F., BENEDETTINI M., et al.
2004ApJ...605..259P viz 118 33 X-rays from HH 80, HH 81, and the central region. PRAVDO S.H., TSUBOI Y. and MAEDA Y.
2006A&A...453.1003T viz 417 88 A SCUBA imaging survey of ultracompact HII regions. The environments of massive star formation. THOMPSON M.A., HATCHELL J., WALSH A.J., et al.
2008AJ....135.1708B 113           X         3 24 18 The ionizing stars of the galactic ultra-compact H II region G45.45+0.06. BLUM R.D. and McGREGOR P.J.
2009ApJ...690..850P 394       D     X C F     9 54 8 GGD 27: X-rays from a massive protostar with an outflow. PRAVDO S.H., TSUBOI Y., SUZUKI Y., et al.
2009ApJS..182..143M viz 182 170 The legacy of SCUPOL: 850 µm imaging polarimetry from 1997 to 2005. MATTHEWS B.C., McPHEE C.A., FISSEL L.M., et al.
2009PABei..27..316C 27 0 Near-infrared polarimetry in study of star formation. CHEN Z.-W. and JIANG Z.-B.
2016ApJ...824...95K viz 2312     A S   X C       56 14 3 Near-infrared imaging polarimetry of GGD 27: circular polarization and magnetic field structures. KWON J., TAMURA M., HOUGH J.H., et al.
2022ApJ...926....6T 45           X         1 6 3 Polarization Spectrum of Near-Infrared Zodiacal Light Observed with CIBER. TAKIMOTO K., ARAI T., MATSUURA S., et al.

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