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Akademický článek
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Autor:
Shenar, T., Oskinova, L., Hamann, W. -R., Corcoran, M. F., Moffat, A. F. J., Pablo, H., Richardson, N. D., Waldron, W. L., Huenemoerder, D. P., Apell��niz, J. Ma��z, Nichols, J. S., Todt, H., Naz��, Y., Hoffman, J. L., Pollock, A. M. T., Negueruela, I.
Eclipsing systems of massive stars allow one to explore the properties of their components in great detail. We perform a multi-wavelength, non-LTE analysis of the three components of the massive multiple system $��$ Ori A, focusing on the fundame
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::6e1c90d5fd8ddb92262b39e709565012
Autor:
Nichols, J. S., Huenemoerder, D. P., Corcoran, M. F., Waldron, W., Naz��, Y., Pollock, A. M. T., Moffat, A. F. J., Lauer, J., Shenar, T., Russell, C. M. P., Richardson, N. D., Pablo, H., Evans, N R., Hamaguchi, K., Gull, T., Hamann, W. R., Oskinova, L., Ignace, R., Hoffman, Jennifer L., Hole, K. T., Lomax, J. R.
We present time-resolved and phase-resolved variability studies of an extensive X-ray high-resolution spectral dataset of the $��$ Orionis Aa binary system. The four observations, obtained with Chandra ACIS HETGS, have a total exposure time of ~4
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::c8aeb3ed993067788722b8df9822af52
Context. Zeta Pup is the X-ray brightest O-type star of the sky. This object was regularly observed with the RGS instrument aboard XMM-Newton for calibration purposes, leading to an unprecedented set of high-quality spectra. Aims. We have previously
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::9508323532604eaa6cbc6b2d8f4c0d8a
During recent years some non-thermal radio emitting OB stars have been discovered to be binary, or multiple systems. The non-thermal emission is due to synchrotron radiation that is emitted by electrons accelerated up to high energies. The electron a
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::92a77be2fe475c361907f52610b36c24
http://arxiv.org/abs/1110.2622
http://arxiv.org/abs/1110.2622
Autor:
Wade, G. A., Grunhut, J. H., Marcolino, W. L. F., Martins, F., Howarth, I., Naz��, Y., Walborn, N., Collaboration, the MiMeS
Only 5 Of?p stars have been identified in the Galaxy. Of these, 3 have been studied in detail, and within the past 5 years magnetic fields have been detected in each of them. The observed magnetic and spectral characteristics are indicative of organi
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::b437cc42084c017c7e8ea4ebf94fb23b
Akademický článek
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Publikováno v:
In European Neuropsychopharmacology October 2014 24 Supplement 2:S172-S172
Publikováno v:
Monthly Notices of the Royal Astronomical Society; 5/11/2005, Vol. 359 Issue 2, p688-698, 11p
Publikováno v:
Astronomy and Astrophysics; December 2009, Vol. 508 Issue: 2 p805-821, 17p