The peculiar southern H II region RCW 34

Details The peculiar southern H II region RCW 34 The peculiar southern H II region RCW 34

Aug 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988a%26a...202..240h&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 202, no. 1-2, Aug. 1988, p. 240-252.

Astronomy and Astrophysics

Astrophysics

14

Astronomical Spectroscopy, Galactic Radiation, H Ii Regions, Southern Sky, Brightness, Charge Coupled Devices, Interstellar Matter, O Stars, Ubv Spectra

Scientific paper

CCD imaging and spectroscopy, UBV photometry, and astrometric measurements are reported for the Galactic H II region RCW 34, which appears to be a nebula with vBH 25a as its exciting star. The data are presented in extensive tables, graphs, and sample images and spectra and discussed in detail. A 100-km/s feature is identified as an ionization front, and it is shown that a new star is forming in a molecular cloud behind this front. The exciting star is classified as a ZAMS star of type O8.5V, at a distance of 2.9 kpc.

Affiliated with

Also associated with

No associations

Rating

The peculiar southern H II region RCW 34 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 The peculiar southern H II region RCW 34, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The peculiar southern H II region RCW 34 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1693113