Based on data from MOST, a Canadian Space Agency mission operated by Microsat Systems Canada Inc. (formerly the space division of Dynacon, Inc.) and the University of Toronto Institute for Aerospace Studies and the University of British Columbia, with the assistance of the University of Vienna.
New slowly pulsating B stars in the field of the young open cluster NGC 2244 discovered by the MOST photometric satellite★
Article first published online: 28 NOV 2011
© 2011 The Authors Monthly Notices of the Royal Astronomical Society © 2011 RAS
Monthly Notices of the Royal Astronomical Society
Volume 420, Issue 1, pages 291–298, February 2012
How to Cite
Gruber, D., Saio, H., Kuschnig, R., Fossati, L., Handler, G., Zwintz, K., Weiss, W. W., Matthews, J. M., Guenther, D. B., Moffat, A. F. J., Rucinski, S. M. and Sasselov, D. (2012), New slowly pulsating B stars in the field of the young open cluster NGC 2244 discovered by the MOST photometric satellite. Monthly Notices of the Royal Astronomical Society, 420: 291–298. doi: 10.1111/j.1365-2966.2011.20033.x
- Issue published online: 23 JAN 2012
- Article first published online: 28 NOV 2011
- Accepted 2011 October 18. Received 2011 October 17; in original form 2011 June 21
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