The deep luminosity function of the globular cluster M30

Details The deep luminosity function of the globular cluster M30 The deep luminosity function of the globular cluster M30

Feb 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990apj...350..662p&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 350, Feb. 20, 1990, p. 662-671. Research supported by the Fondazione Ingegn

Astronomy and Astrophysics

Astrophysics

29

Globular Clusters, Metallicity, Stellar Evolution, Stellar Luminosity, Astronomical Photometry, Color-Magnitude Diagram, Stellar Mass

Scientific paper

An effort is made to determine the mass function in low-metallicity, postcore-collapse globular cluster M30, as well as to analyze its radial trend, using new deep CCD photometry. It is confirmed that oxygen-enhanced isochrones yield a good representation of the color-magnitude diagrams. Luminosity functions are constructed and corrected for for field-object contamination and incompleteness. The data presented agree with the power-law trend ascertained by Pryor et al. (1986) for a multimass King-Michie model, yielding a global slope of 0.7.

Affiliated with

Also associated with

No associations

Rating

The deep luminosity function of the globular cluster M30 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 deep luminosity function of the globular cluster M30, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The deep luminosity function of the globular cluster M30 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1841490