High latitude molecular clouds - Distances derived from accurate photometry

Details High latitude molecular clouds - Distances derived from accurate photometry High latitude molecular clouds - Distances derived from accurate photometry

Oct 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989a%26a...223..313f&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 223, no. 1-2, Oct. 1989, p. 313-320. Research supported by the Danish Board fo

Astronomy and Astrophysics

Astrophysics

49

Astronomical Photometry, Molecular Clouds, Nebulae, A Stars, Astronomical Catalogs, B Stars, Carbon Monoxide, H Beta Line, Interstellar Extinction

Scientific paper

Four-color uvby and H-beta photometry for 237SAO stars earlier than G0 is used to estimate the color excesses and distribution toward five areas containing high latitude molecular clouds. For three areas, the color excesses indicate the existence of a rather large interstellar absorption, which can be attributed to the dust material associated with the molecular clouds. Based on the mean photometric error of one star, color excesses and distances are obtained with a mean accuracy of 0.016 m and 20 percent, respectively.

Affiliated with

Also associated with

No associations

Rating

High latitude molecular clouds - Distances derived from accurate photometry 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 High latitude molecular clouds - Distances derived from accurate photometry, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and High latitude molecular clouds - Distances derived from accurate photometry will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1527005