Zobrazeno 1 - 10
of 36
pro vyhledávání: '"S. A. Ilovaisky"'
Autor:
Lydie Koch-Miramond, P. A. Charles, Tim Naylor, S. A. Ilovaisky, Bruce Margon, L. van Zyl, Z. Ioannou
Publikováno v:
Astronomy & Astrophysics. 399:211-218
We present HST UV observations of the high-inclination low mass X-ray binary AC211 (X2127+119), which is located in the globular cluster M15 (NGC 7078). We have discovered a C P Cygni profile in this system, which confirms the existence of an o
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::b6503950e15670f8a5255fb58317f9b9
https://doi.org/10.1051/0004-6361:20021578
https://doi.org/10.1051/0004-6361:20021578
Autor:
Danuta Sosnowska, D. Gillet, A. Laloge, S. A. Ilovaisky, Denis Mégevand, François Bouchy, J.-C. Brunel, P. E. Blanc, M. Merzougui, Jean-Pierre Meunier, D. Kohler, Pierre Richaud, A. Point, X. Regal, Y. Richaud, P. Vors, Francesco Pepe, L. Hill, S. Perruchot, Jerome Schmitt, H. Le Coroller, R. Sottile, G. Knispel, Gabriel Moreaux, M. Fleury, C. Carol
Publikováno v:
SPIE Proceedings.
SOPHIE is a new fiber-fed echelle spectrograph in operation since October 2006 at the 1.93-m telescope of Observatoire de Haute-Provence. Benefiting from experience acquired on HARPS (3.6-m ESO), SOPHIE was designed to obtain accurate radial velociti
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::386b770da7ac9361bbb1ac4c34b5d8d6
https://doi.org/10.1117/12.787379
https://doi.org/10.1117/12.787379
Autor:
Areg M. Mickaelian, S. K. Balayan, M.-P. Veron-Cetty, S. A. Ilovaisky, P. Veron, C. Chevalier
We report the discovery of a new bright (V$\sim$12.6) cataclysmic variable star identified with the ROSAT X-ray source RX J1643.7+3402. Spectroscopic and photometric observations show it to be a novalike variable sharing some of the characteristics o
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::fdcc9fd3d9f8d6f2c1ec105c914d7188
Autor:
C. Chevalier, J. L. Atteia, Michel Boer, J. F. Olive, S. A. Ilovaisky, Holger Pedersen, M. Niel, C. Barat
Publikováno v:
AIP Conference Proceedings.
TAROT (Telescope a Action Rapide pour les Objets Transitoires) is a two step project whose goal is the observation of short optical transient sources, primarily GRBs. As a first step, a CCD camera will be used at the focus of a 25 cm telescope, able
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::9eaeaaaf65c39621d7c28b2cf9529c4e
https://doi.org/10.1063/1.51575
https://doi.org/10.1063/1.51575
Publikováno v:
Astrophysical Journal, 361(1), 590-595. IOP Publishing Ltd.
This paper describes the optical identification and the X-ray light curve of an ultrashort transient X-ray source, GS 1354 - 64, discovered on February 13, 1987 by the All Sky Monitor (ASM) on onboard Ginga satellite. The data obtained by ASM are sup
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::8001b9139fe5b7657cccdb28aadbb777
https://dare.uva.nl/personal/pure/en/publications/outburst-identification-and-xray-light-curve-of-gs-135464--mx-135364-centaurus-x2(908847a4-03a2-42bc-9c26-b2944eb046e5).html
https://dare.uva.nl/personal/pure/en/publications/outburst-identification-and-xray-light-curve-of-gs-135464--mx-135364-centaurus-x2(908847a4-03a2-42bc-9c26-b2944eb046e5).html
Autor:
S A Ilovaisky
Publikováno v:
Physica Scripta. :78-86
X-ray, optical and ultraviolet observations of massive binary systems have yielded basic information on the masses and radii of the massive early-type companions and the masses and moments of inertia of the neutron stars. We briefly review the eviden
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::6a376bfd743f94440330ed9579a55016
https://doi.org/10.1088/0031-8949/1984/t7/018
https://doi.org/10.1088/0031-8949/1984/t7/018
Publikováno v:
Space Science Reviews. 40:219-224
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::2c77afecb142ce0c1ebbba82577bac46
https://doi.org/10.1007/bf00212888
https://doi.org/10.1007/bf00212888
Publikováno v:
Symposium - International Astronomical Union. 98:151-154
Analysis of optical spectra of HD102567 (HEN 715), the optical counterpart of the X-ray source 4U1145-61 is presented. Estimates of the star's rotation velocity, inclination angle, distance and envelope characteristics are given. Some consequences of
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::3ef5573f64256bee15763b7362371a77
https://doi.org/10.1017/s0074180900037724
https://doi.org/10.1017/s0074180900037724
Autor:
Tim Naylor, Keith O. Mason, R. H. D. Corbet, S. A. Ilovaisky, Arvind Parmar, J. van Paradijs, Christian Motch, M. van der Klis, A. P. Smale, K. Mukai, P. A. Charles
Publikováno v:
Monthly Notices of the Royal Astronomical Society, 233, 51-63. Oxford University Press
La campagne d'observation internationale de CAL 83, en 1984, a permis la determination sans aucune ambiguite de la periode de cette binaire RX. Elle est de 1.04 jours avec une modulation sinusoidale de 0,22 mag autour d'une valeur moyenne V=16.87. Oc
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::42031a22141c4adb43f34363b22f461d
https://doi.org/10.1093/mnras/233.1.51
https://doi.org/10.1093/mnras/233.1.51
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 176:91-102
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::155b5496eb006310eb500ff4b594dff0
https://doi.org/10.1093/mnras/176.1.91
https://doi.org/10.1093/mnras/176.1.91