X-rays from the open cluster NGC 6633
Abstract
NGC 6633 is a young, open cluster with a similar age to the Hyades and Praesepe, but probably a lower metallicity. We present the results of ROSAT High Resolution Imager observations of an optically selected catalogue of likely members of NGC 6633. 8 out of 51 NGC 6633 members have been detected, with main-sequence spectral types A to G, above a threshold X-ray luminosity of ~6-12×1028ergs-1. We find that NGC 6633 does not contain cool stars that are as X-ray luminous as the most active objects in the Hyades and that the median X-ray luminosity of F-G stars in NGC 6633 is less than that in the Hyades, but probably greater than in Praesepe. However, when X-ray activity is expressed as the X-ray to bolometric flux ratio we find that NGC 6633 and the Hyades are very similar and display similar peak levels of coronal activity. We attribute this discrepancy to a number of possible wide binary systems with higher X-ray (and bolometric) luminosities in the Hyades sample and either a low metallicity in NGC 6633, which makes its cool stars both X-ray and bolometrically less luminous at the same colour, or a distance to NGC 6633 that has been underestimated, which would decrease stellar X-ray luminosities without changing X-ray to bolometric flux ratios.
- Publication:
-
Monthly Notices of the Royal Astronomical Society
- Pub Date:
- June 2001
- DOI:
- 10.1046/j.1365-8711.2001.04342.x
- Bibcode:
- 2001MNRAS.324..473H
- Keywords:
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- STARS: LATE-TYPE;
- STARS: ROTATION;
- OPEN CLUSTERS AND ASSOCIATIONS: INDIVIDUAL: NGC 6633;
- X-RAYS: STARS