The spectrographs on-board the World Space Observatory (WSO) will provide access to the 1020-1800 Å wavelength range with unprecedented sensitivity. Previous observatories operating in the 1150-2000 Å range (such as IUE and HST-STIS) have proved extremely useful to study the winds of OB type stars, which leave their most prominent imprints in the
Esta sección ofrece el acceso a la base de datos de Publicaciones que recopila los artículos del IAC publicados en revistas científicas. Por favor, pulsa la flecha del menú para ver todas las opciones de búsqueda y de ordenación de resultados; autor, revista, año, etc..
Además ofrece acceso al repositorio de preprints del IAC: https://research.iac.es/preprints/l
-
WSO and the winds of massive stars: the gate to the metal-poor Local UniverseGarcia, M. et al.92011
-
X-ray and Optical Observations of 4U2129+47=V1727Cyg in a Low State
Not Available
Garcia, M. R.Fecha de publicación:
91992 -
X-ray Binary Jets: New Constraints From Multi-wavelength Spectroscopy And Rapid Timing
Optical instruments for measurement of precise rapid timing have recently given us the capability of going beyond X-ray variability. Observations of several sources have revealed multi-wavelength variations on a wide range of continuous timescales from ms up, and intriguing flux correlations with X-ray fluctuations have been found. These give
Gandhi, Poshak et al.Fecha de publicación:
92011 -
X-ray re-brightening detected from the neutron star transient XTE J1701-407
Following our recent report on the transition to quiescence of the transient neutron star low-mass X-ray binary XTE J1701-407 (ATel #3604), we continued to monitor the source in X-rays. Further observations were carried out between August 31 and September 20, during which Swift pointed towards the source once every 2-4 days with the XRT operated in
Degenaar, N. et al.Fecha de publicación:
92011 -
X-ray spectra of the RIXOS source sample
We present results of an extensive study of the X-ray spectral properties of sources detected in the RIXOS survey, which is a large, nearly complete sample of objects detected serendipitously in ROSAT PSPC fields down to a flux limit of 3x10^-14ergcm^-2s^-1 (0.5-2keV). We show that for X-ray surveys containing sources with low count rate, such as
Mittaz, J. P. D. et al.Fecha de publicación:
91999 -
X-ray spectral variability of LINERs selected from the Palomar sample
Context. Variability is a general property of active galactic nuclei (AGN). The way in which these changes occur at X-rays is not yet clearly understood. In the particular case of low-ionization nuclear emission line region (LINER) nuclei, variations on the timescales from months to years have been found for some objects, but the main driver of
Hernández-García, L. et al.Fecha de publicación:
92014