A new, compact far-infrared source in the W31 region

1978 ◽  
Vol 221 ◽  
pp. L77 ◽  
Author(s):  
G. G. Fazio ◽  
C. J. Lada ◽  
D. E. Kleinmann ◽  
E. L. Wright ◽  
P. T. P. Ho ◽  
...  
Keyword(s):  
Far Infrared ◽  
Infrared Source

Near-infrared observations of the far-infrared source V region in NGC 6334

1982 ◽  
Vol 258 ◽  
pp. 165 ◽  
Author(s):  
J. Fischer ◽  
R. R. Joyce ◽  
M. Simon ◽  
T. Simon
Keyword(s):  
Near Infrared ◽  
Far Infrared ◽  
Infrared Source ◽  
Infrared Observations ◽  
V Region ◽  
Ngc 6334

Evidence for a variable far-infrared source in NGC 6334

1979 ◽  
Vol 232 ◽  
pp. L183 ◽  
Author(s):  
B. McBreen ◽  
G. G. Fazio ◽  
M. Stier ◽  
E. L. Wright
Keyword(s):  
Far Infrared ◽  
Infrared Source ◽  
Ngc 6334

scholarly journals Near-Infrared Images of the Serpens Molecular Cloud Core

1989 ◽  
Vol 120 ◽  
pp. 227-230
Author(s):  
C. Eiroa ◽  
M. Casali
Keyword(s):  
Molecular Cloud ◽  
Large Scale ◽  
Near Infrared ◽  
Far Infrared ◽  
Infrared Images ◽  
Infrared Source ◽  
Stellar Objects ◽  
Dark Clouds ◽  
First Time ◽  
Cloud Core

ABSTRACT:Near-infrared images of the Serpens molecular cloud core have been carried out at UKIRT (Mauna Kea Observatory) using the infrared array camera, IRCAM. A large-scale diffuse nebulosity extending over the central part of the core is observed. Over 100 K-sources are detected in the 30 arc min2 cloud core. Some of them are PMS objects which were previously unknown. For the first time, a near-infrared counterpart of the far-infrared source Seroens FIRS1 has been detected. The 2.2 µm source appears as a point like object at the apex of an extended knotty, jet-like nebulosity oriented towards the northwest. In addition, a group of 11 stellar objects is seen in the position of the IR/radio source SVS4. These objects are embedded in a very faint nebulosity and form one of the densest clustering of young stars found in dark clouds.

scholarly journals Constraints on Far-Infrared Source Counts in the Lockman Hole using a Power Spectrum Analysis

2001 ◽  
Vol 204 ◽  
pp. 301-301
Author(s):  
H. Matsuhara ◽  
K. Kawara ◽  
Y. Sofue ◽  
Y. Taniguchi ◽  
Y. Sato ◽  
...  
Keyword(s):  
Background Radiation ◽  
Power Spectra ◽  
Far Infrared ◽  
Infrared Space Observatory ◽  
Infrared Source ◽  
Star Forming ◽  
The Galaxy ◽  
Galaxy Count ◽  
Infrared Background ◽  
Lockman Hole

We present the characteristics of far-infrared (FIR) brightness fluctuations at 90 μm and 170 μm in the Lockman Hole, which were surveyed with the ISOPHOT instrument aboard the Infrared Space Observatory (ISO), and give constraints on the galaxy number counts down to 30 mJy at 90 μm and 50 mJy at 170 μm. The fluctuation power spectra of the FIR images are not dominated by IR cirrus, and are instead most likely due to star-forming galaxies. This analysis indicates the existence of strong evolution in the counts. Especially at 90 μm, the source density is much larger than that expected from the currently available galaxy count models. The galaxies responsible for the fluctuations also significantly contribute to the cosmic infrared background radiation recently derived from an analysis of the COBE data.

Discovery of a compact far-infrared source, IR 12.4+0.5

1979 ◽  
Vol 228 ◽  
pp. 439
Author(s):  
E. L. Wright ◽  
W. Decampli ◽  
G. G. Fazio ◽  
C. J. Lada ◽  
F. J. Low ◽  
...  
Keyword(s):  
Far Infrared ◽  
Infrared Source

scholarly journals Detection of H2O Emission from the Far-infrared Source AFCRL (UOA) 19

1975 ◽  
Vol 170 (1) ◽  
pp. 37P-38P ◽  
Author(s):  
G. J. White ◽  
L. T. Little ◽  
E. A. Parker ◽  
P. S. Nicholson ◽  
G. H. MacDonald ◽  
...  
Keyword(s):  
Far Infrared ◽  
Infrared Source
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