IRAS Sources behind the Solar circle (Wouterloot+ 1989)

Details IRAS Sources behind the Solar circle (Wouterloot+ 1989) IRAS Sources behind the Solar circle (Wouterloot+ 1989)

Sep 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994ycat..40800149w&link_type=abstract

VizieR On-line Data Catalog: J/A+AS/80/149. Originally published in: 1989A&AS...80..149W

Computer Science

Infrared Sources, Co, Galactic Plane, Radio Lines

Scientific paper

CO (J=1->0) has been observed with the 15-m SEST and the 30-m IRAM telescope in the direction of 1302 IRAS sources with colors of star forming regions located within 10 deg of the galactic plane in the interval between 85 and 280 deg. Emission components with line profiles that are non-Gaussian (showing, e.g., possible self-absorption or wings) are identified; this information may serve as a basis for selecting sources for future research. For all components, kinematic heliocentric and galactocentric distances, and distances from the galactic plane are derived. For those components which may be associated with the IRAS sources, bolometric luminosities are derived. These data will be analyzed and compared with HI data in subsequent papers. (1 data file).

Affiliated with

Also associated with

No associations

Rating

IRAS Sources behind the Solar circle (Wouterloot+ 1989) 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 IRAS Sources behind the Solar circle (Wouterloot+ 1989), we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and IRAS Sources behind the Solar circle (Wouterloot+ 1989) will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1713896