SIMBAD references

2004A&A...421..175P - Astronomy and Astrophysics, volume 421, 175-186 (2004/7-1)

XMM-Newton observations of the young open cluster Blanco1. I. X-ray spectroscopy and photometry.

PILLITTERI I., MICELA G., SCIORTINO S., DAMIANI F. and HARNDEN F.R.Jr

Abstract (from CDS):

We present an X-ray study of the high metallicity young open cluster Blanco 1 based on XMM-Newton data. X-ray spectroscopy of cluster members is presented for the first time as well as new X-ray distribution functions of late-type stars. We detected all known dF and dG stars in the EPIC field and 80% and 90% of dK and dM stars, respectively. The X-ray spectral analysis of the X-ray brightest cluster stars and X-ray color analysis of a larger sample show that a model with two temperatures (at about 0.3 and 1keV) explains the quiescent activity phase spectra. We discuss also the nature of unidentified X-ray sources in the observed region and their X-ray spectral properties.

Abstract Copyright:

Journal keyword(s): X-ray: stars - stars: activity - Galaxy: open clusters and associations: individual: Blanco 1

VizieR on-line data: <Available at CDS (J/A+A/421/175): tablea1.dat tableb1.dat>

Nomenclature: Table 1: [PMS2004] AN (Nos P1-P8). Table A1: [PMS2004] Opt NNN N=90 among (Nos 2-190). Table B1: [PMS2004] Un NN (Nos 1-64).

CDS comments: The electronic-only appendix is referred to as Appendix B in the text, Table A.1 and Figures A.1 and A.2 in this second appendix should be Table B.1 (which is different from Table A.1 in Appendix A p. 184), Figures B.1 and B.2(.)

Simbad objects: 209

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2020.12.05-16:48:30

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