A Multiwavelength Study of the Galactic Star Forming Region Associated with IRAS 20255+3712 / S 106

Details A Multiwavelength Study of the Galactic Star Forming Region Associated with IRAS 20255+3712 / S 106 A Multiwavelength Study of the Galactic Star Forming Region Associated with IRAS 20255+3712 / S 106

Mar 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003basi...31..391g&link_type=abstract

Bulletin of the Astronomical Society of India, vol. 31, p.391-393

Mathematics

Logic

2

Scientific paper

The Galactic star forming region associated with IRAS 20255+3712 / S 106 has been mapped simultaneously in 150 and 210 μm bands using the TIFR 1-metre balloon borne far-infrared (FIR) telescope with an angular resolution of 1 arc min. The presence of a disk of cold dust is inferred from these FIR maps. High sensitivity and angular resolution radio continuum imaging at 325, 610 and 1280 MHz carried out using the Giant Metrewave Radio Telescope (GMRT), demonstrates the morphological contrast between the emission from the ionized gas and the thermal dust emission. The emission from the carriers of Unidentified Infrared Bands (UIBs) in the mid infrared 6-9 μm as extracted from the Midcourse Satellite Experiment (MSX) survey (at 8, 12, 14 and 21 μm), compares rather well with the radio emission. 23

Affiliated with

Also associated with

No associations

Rating

A Multiwavelength Study of the Galactic Star Forming Region Associated with IRAS 20255+3712 / S 106 does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with A Multiwavelength Study of the Galactic Star Forming Region Associated with IRAS 20255+3712 / S 106, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and A Multiwavelength Study of the Galactic Star Forming Region Associated with IRAS 20255+3712 / S 106 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1882060