The Internal Structure of the M31 Globular Cluster G302

Details The Internal Structure of the M31 Globular Cluster G302 The Internal Structure of the M31 Globular Cluster G302

May 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993aas...182.5013h&link_type=abstract

American Astronomical Society, 182nd AAS Meeting, #50.13; Bulletin of the American Astronomical Society, Vol. 25, p.885

Astronomy and Astrophysics

Astronomy

1

Scientific paper

We have used the CFHT's HRCam to obtain V- and I-band photometry of approximately two dozen M31 globular clusters under conditions of excellent seeing (/lineFWHM =~ 0.('') 6 =~ 2.1 pc). Seeing convolved Michie--King models are being fit to the surface brightness profiles of these clusters in order to determine their tidal radii and to constrain the distribution of cluster central concentrations in the M31 system. This paper presents preliminary results for G302, a bright cluster located ~ 32('') SE of the nucleus of M31. Our fit suggests that G302 has a central concentration of c =~ 2, a core radius of r_c =~ 1 pc and a tidal radius of r_t =~ 100 pc.

Affiliated with

Also associated with

No associations

Rating

The Internal Structure of the M31 Globular Cluster G302 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 Internal Structure of the M31 Globular Cluster G302, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The Internal Structure of the M31 Globular Cluster G302 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1849566