UBVR CCD photometry of stars in M31. II - Five disk fields

Details UBVR CCD photometry of stars in M31. II - Five disk fields UBVR CCD photometry of stars in M31. II - Five disk fields

Jun 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988apj...329..651h&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 329, June 15, 1988, p. 651-686.

Astronomy and Astrophysics

Astrophysics

40

Andromeda Galaxy, Charge Coupled Devices, Interstellar Matter, Spiral Galaxies, Star Formation, Stellar Spectrophotometry, Ubv Spectra, Color-Magnitude Diagram, H I Regions, H Ii Regions, Stellar Luminosity, Tables (Data)

Scientific paper

Deep CCD photometry of five fields in the disk of M31 provide comparisons for different positions and environments. Only marginally different recent star-formation histories are indicated by the maximum brightness levels and luminosity functions of the main sequences. Mean reddenings range from 0.13 to 0.38. The reddening varies with distance from the nucleus, following the relation previously found for H I density and for reddenings in H II regions, with a maximum at ≡10 kpc from the center.

Affiliated with

Also associated with

No associations

Rating

UBVR CCD photometry of stars in M31. II - Five disk fields 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 UBVR CCD photometry of stars in M31. II - Five disk fields, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and UBVR CCD photometry of stars in M31. II - Five disk fields will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1177820