[en] The key empirical property of the X-ray emission from O stars is a strong correlation between the bolometric and X-ray luminosities. In the framework of the Chandra Carina Complex Project, 129 O and B stars have been detected as X-ray sources; 78 of those, all with spectral type earlier than B3, have enough counts for at least a rough X-ray spectral characterization. This leads to an estimate of the L [SUB]X[/SUB]-L [SUB]BOL[/SUB] ratio for an exceptional number of 60 O stars belonging to the same region and triples the number of Carina massive stars studied spectroscopically in X-rays. The derived log(L [SUB]X[/SUB]/L [SUB]BOL[/SUB]) is -7.26 for single objects, with a dispersion of only 0.21 dex. Using the properties of hot massive stars listed in the literature, we compare the X-ray luminosities of different types of objects. In the case of O stars, the L [SUB]X[/SUB]-L [SUB]BOL[/SUB] ratios are similar for bright and faint objects, as well as for stars of different luminosity classes or spectral types. Binaries appear only slightly harder and slightly more luminous in X-rays than single objects; the differences are not formally significant (at the 1% level), except for the L [SUB]X[/SUB]-L [SUB]BOL[/SUB] ratio in the medium (1.0-2.5 keV) energy band. Weak-wind objects have similar X-ray luminosities but they display slightly softer spectra compared with "normal" O stars with the same bolometric luminosity. Discarding three overluminous objects, we find a very shallow trend of harder emission in brighter objects. The properties of the few B stars bright enough to yield some spectral information appear to be different overall (constant X-ray luminosities, harder spectra), hinting that another mechanism for producing X-rays, besides wind shocks, might be at work. However, it must be stressed that the earliest and X-ray brightest among these few detected objects are similar to the latest O stars, suggesting a possibly smooth transition between the two processes.
Disciplines :
Space science, astronomy & astrophysics
Author, co-author :
Nazé, Yaël ; Université de Liège - ULiège > Département d'astrophys., géophysique et océanographie (AGO) > Astrophysique observationnelle (sol et espace)
Broos, P. S.; Department of Astronomy & Astrophysics, 525 Davey Laboratory, Pennsylvania State University, University Park, PA 16802, USA
Oskinova, L.; Institute for Physics and Astronomy, Universität Potsdam, 14476 Potsdam, Germany
Townsley, L. K.; Department of Astronomy & Astrophysics, 525 Davey Laboratory, Pennsylvania State University, University Park, PA 16802, USA
Cohen, D.; Swarthmore College Department of Physics and Astronomy, 500 College Avenue, Swarthmore, PA 19081, USA
Corcoran, M. F.; CRESST and X-ray Astrophysics Laboratory, NASA/GSFC, Greenbelt, MD 20771, USA ; Universities Space Research Association, 10211 Wincopin Circle, Suite 500 Columbia, MD 21044, USA
Evans, N. R.; Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138, USA
Gagné, M.; Department of Geology and Astronomy, West Chester University, West Chester, PA 19383, USA
Moffat, A. F. J.; Département de Physique, Université de Montréal, Succursale Centre-Ville, Montréal, QC, H3C 3J7, Canada ; Centre de recherche en astrophysique du Québec, Canada
Pittard, J. M.; School of Physics and Astronomy, The University of Leeds, Leeds LS2 9JT, UK
Rauw, Grégor ; GAPHE, Département AGO, Université de Liège, Allée du 6 Août 17, Bat. B5C, B4000 Liège, Belgium
ud-Doula, A.; Penn State Worthington Scranton, 120 Ridge View Drive, Dunmore, PA 18512, USA
Walborn, N. R.; Space Telescope Science Institute, 3700 Martin Drive, Baltimore, MD 21218, USA
Sanz-Forcada, J., Franciosini, E., & Pallavicini, R. 2004, A&A, 421, 715
Seward, F. D., Forman, W. R., Giacconi, R., Griffiths, R. E., Harnden, F. R., Jr., Jones, C., & Pye, J. P. 1979, ApJ, 234, L55
Skiff, B. A. 2009, Catalogue of Stellar Spectral Classifications, VizieR Catalog B/mk/mktypes (Lowell Observatory), 1, 2023
Smith, R. K., Brickhouse, N. S., Lieadhl, D. A., & Raymond, J. C. 2001, ApJ, 556, L91
Stelzer, B., Flaccomio, E., Montmerle, T., Micela, G., Sciortino, S., Favata, F., Preibisch, T., & Feigelson, E. D. 2005, ApJS, 160, 557
Townsley, L. K., Feigelson, E. D., Montmerle, T., Broos, P. S., Chu, Y.-H., & Garmire, G. P. 2003, ApJ, 593, 874
Townsley, L. K. et al. 2011, ApJS, 194, 1, (CCCP Intro Paper)
ud-Doula, A. & Owocki, S. P. 2002, ApJ, 576, 413
ud-Doula, A., Townsend, R. H. D., & Owocki, S. P. 2006, ApJ, 640, L191
Vink, J. S., de Koter, A., & Lamers, H. J. G. L. M. 2000, A&A, 362, 295
Vuong, M. H., Montmerle, T., Grosso, N., Feigelson, E. D., Verstraete, L., & Ozawa, H. 2003, A&A, 408, 581
Walborn, N. R. 1995, RevMexAA Conf. Ser., 2, 51
Walborn, N. R. 2009, Massive Stars from Pop. III and GRBS to the Milky Way (STScI Symp. Ser. 20), ed. M. Livio & E. Villaver (Cambridge: Cambridge Univ. Press), 167
Walborn, N. R., Nichols, J. S., & Waldron, W. L. 2009, ApJ, 703, 633
Wang, J., Townsley, L. K., Feigelson, E. D., Broos, P. S., Getman, K. V., Romn-Z̃iga, C. G., & Lada, E. 2008, ApJ, 675, 464
Wilms, J., Allen, A., & Mc Cray, R. 2000, ApJ, 542, 914