CO and optical observations of the Magellanic Bridge

Details CO and optical observations of the Magellanic Bridge CO and optical observations of the Magellanic Bridge

Nov 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000a%26a...363..451s&link_type=abstract

Astronomy and Astrophysics, v.363, p.451-454 (2000)

Astronomy and Astrophysics

Astrophysics

7

Galaxies: Ism, Galaxies: Magellanic Clouds, Galaxies: Photometry, Radio Lines: Galaxies, Radio Lines: Ism

Scientific paper

We present 12CO(1-0) molecular line and BV CCD observations towards 0311-7651, a region in the Magellanic Bridge where cold atomic Hydrogen has previously been detected by Kobulnicky & Dickey. Additionally, BV images of a comparison field 1deg to the South were taken. No CO was detected to a limit of ~ 0.06 Kelvin, and the colour-magnitude diagrams show no evidence for a stellar association in either field. Based on observations made with the Danish 1.54-m and SEST telescopes at the European Southern Observatory, La Silla, Chile.

Affiliated with

Also associated with

No associations

Rating

CO and optical observations of the Magellanic Bridge 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 CO and optical observations of the Magellanic Bridge, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and CO and optical observations of the Magellanic Bridge will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1146890