The X-ray Luminosity Distributions of the high-metallicity open cluster Blanco 1

Details The X-ray Luminosity Distributions of the high-metallicity open cluster Blanco 1 The X-ray Luminosity Distributions of the high-metallicity open cluster Blanco 1

Mar 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003a%26a...399..919p&link_type=abstract

Astronomy and Astrophysics, v.399, p.919-929 (2003)

Astronomy and Astrophysics

Astrophysics

14

X-Ray: Stars, Stars: Activity, Open Clusters And Associations: Individual: Blanco 1

Scientific paper

We present X-ray Luminosity Distributions (XLDs) of late-type members (dF, dG, dK, dM) of the Blanco 1 cluster, based on ROSAT-HRI data and new astrometric-photometric membership obtained from the GSC-II project. For the first time we present the XLD of dM stars of this cluster. The high metallicity of Blanco 1 allows us to investigate the role of chemical composition on the coronal emission of late-type stars. Comparison between X-ray Luminosity Distributions of Blanco 1 and Pleiades, NGC 2516 and alpha Per suggests a possible metallicity effect in dM stars.

Affiliated with

Also associated with

No associations

Rating

The X-ray Luminosity Distributions of the high-metallicity open cluster Blanco 1 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 X-ray Luminosity Distributions of the high-metallicity open cluster Blanco 1, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The X-ray Luminosity Distributions of the high-metallicity open cluster Blanco 1 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1881393