GSS 30 - an infrared reflection nebula in the Ophiuchus dark cloud

1985 ◽  
Vol 290 ◽  
pp. 261 ◽  
Author(s):  
M. W. Castelaz ◽  
J. A. Hackwell ◽  
G. L. Grasdalen ◽  
R. D. Gehrz ◽  
C. Gullixson
Keyword(s):  
Dark Cloud ◽  
Reflection Nebula ◽  
Infrared Reflection

An infrared reflection nebula surrounding SGS 1 in the NGC 1333 dark cloud

1986 ◽  
Vol 300 ◽  
pp. 406 ◽  
Author(s):  
M. W. Castelaz ◽  
J. A. Hackwell ◽  
G. L. Grasdalen ◽  
R. D. Gehrz
Keyword(s):  
Dark Cloud ◽  
Reflection Nebula ◽  
Infrared Reflection

GSS 30: an Infrared Reflection Nebula in the Ophiuchus Dark Cloud: Erratum

1986 ◽  
Vol 301 ◽  
pp. 502 ◽  
Author(s):  
Michael W. Castelaz ◽  
John A. Hackwell ◽  
Gary L. Grasdalen ◽  
Robert D. Gehrz ◽  
Craig Gullixson
Keyword(s):  
Dark Cloud ◽  
Reflection Nebula ◽  
Infrared Reflection

Deep Imaging Observations of the Lupus 3 Cloud: Dark Cloud Revealed as Infrared Reflection Nebula

2003 ◽  
Vol 125 (3) ◽  
pp. 1407-1417 ◽  
Author(s):  
Yasushi Nakajima ◽  
Tetsuya Nagata ◽  
Shuji Sato ◽  
Takahiro Nagayama ◽  
Chie Nagashima ◽  
...  
Keyword(s):  
Dark Cloud ◽  
Reflection Nebula ◽  
Deep Imaging ◽  
Infrared Reflection

A new CO bipolar flow and dense disk system associated with the infrared reflection nebula GGD 27 IRS

1989 ◽  
Vol 347 ◽  
pp. 894 ◽  
Author(s):  
Takuya Yamashita ◽  
Hiroko Suzuki ◽  
Norio Kaifu ◽  
Motohide Tamura ◽  
Charles M. Mountain ◽  
...  
Keyword(s):  
Disk System ◽  
Reflection Nebula ◽  
Infrared Reflection

The Juggler - A three-lobed near-infrared reflection nebula toward CRL 2136 = OH 17.6 + 0.2

1992 ◽  
Vol 389 ◽  
pp. 357 ◽  
Author(s):  
Joel H. Kastner ◽  
David A. Weintraub ◽  
C. Aspin
Keyword(s):  
Near Infrared ◽  
Reflection Nebula ◽  
Infrared Reflection

scholarly journals Infrared reflection nebula in W75N

1988 ◽  
Vol 233 (4) ◽  
pp. 899-905
Author(s):  
T. Yamashita ◽  
S. Sato ◽  
M. Tamura ◽  
H. Suzuki ◽  
I. Gatley ◽  
...  
Keyword(s):  
Reflection Nebula ◽  
Infrared Reflection

A Near-Infrared Reflection Nebula Associated with NGC 2024 FIR 4

1995 ◽  
Vol 440 ◽  
pp. 722 ◽  
Author(s):  
T. J. T. Moore ◽  
T. Yamashita
Keyword(s):  
Near Infrared ◽  
Reflection Nebula ◽  
Infrared Reflection

scholarly journals Discovery of an extended infrared reflection nebula around S106

1987 ◽  
Vol 225 (2) ◽  
pp. 393-398 ◽  
Author(s):  
I. S. McLean ◽  
M. J. McCaughrean ◽  
I. Gatley ◽  
J. Hough ◽  
S. Sato ◽  
...  
Keyword(s):  
Reflection Nebula ◽  
Infrared Reflection

scholarly journals Herbig–Haro flows around the BBWo 192E (GM 1–23) nebula

2020 ◽  
Vol 498 (4) ◽  
pp. 5109-5115
Author(s):  
T Yu Magakian ◽  
T A Movsessian ◽  
H R Andreasyan ◽  
J Bally ◽  
A S Rastorguev
Keyword(s):  
Star Formation ◽  
Sloan Digital Sky Survey ◽  
Young Stellar Objects ◽  
Infrared Range ◽  
Wide Field ◽  
Proper Motions ◽  
Dark Cloud ◽  
Stellar Objects ◽  
Reflection Nebula ◽  
Sky Survey

ABSTRACT Looking for evidence of recent star formation, we have studied a small comet-shaped reflection nebula, known as BBWo 192E (GM 1–23), which is located in the dark cloud SL 4 in the Vela Molecular Ridge cloud C, and a young infrared cluster embedded into the nebula. We obtained the images of BBWo 192E in Hα and [S ii] lines and in a Sloan Digital Sky Survey i ′ filter with the Blanco telescope at the Cerro Tololo Inter-American Observatory in order to discover new Herbig–Haro (HH) flows. We used the Two-Micron All-Sky Survey and the Wide-field Infrared Survey Explorer to search for additional member stars of the cluster. We also studied the proper motions and parallaxes of the cluster members using GAIA Data Release 2. Five new groups containing at least nine HH objects, tracing several distinct outflows, were revealed. A previously unreported reflection nebula and a number of probable outflow sources were found in the infrared range. The proper motions allowed us to select eight probable member stars in the visual range. Their parallaxes correspond to a mean distance 800 ± 100 pc for this cluster. The bolometric luminosities of the brightest cluster members are 1010 L⊙ (IRAS 08513−4201, the strong source in the centre of the cluster) and 2–6 L⊙ for the five other stars. The existence of optical HH flows around the infrared cluster of young stellar objects suggests that star formation in this cloud is ongoing around the more massive Herbig Ae/Be star. Considering its morphology and other features, this star-forming region is similar to the zone of star formation near CPM 19.

scholarly journals Circumstellar Molecular Gas of the Young Stellar Object SVS 12

1994 ◽  
Vol 140 ◽  
pp. 270-271
Author(s):  
Karl R. Stapelfeldt
Keyword(s):  
Stellar Object ◽  
Class I ◽  
Molecular Gas ◽  
Infrared Source ◽  
Young Stellar Object ◽  
Circumstellar Material ◽  
Reflection Nebula ◽  
Infrared Reflection ◽  
Exciting Star

SVS 12 is an embedded infrared source which is the probable exciting star for HH 12. The source has a “class I” IRAS spectrum and about 20 L© luminosity. Differential reddening between the star (J-K ≥ 6 mag) and the adjacent infrared reflection nebula (J-K= 3 mag) suggests the presence of dense circumstellar material (Stapelfeldt et al. 1991). SVS 12 was observed with the OVRO interferometer in the 13CO 1-0 and CS 2-1 lines and associated continuum, and at the CSO with a bolometer and in the CS 5-4 and CS 7-6 lines.

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