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Radiation-driven winds of hot luminous stars. XIII. A description of NLTE line blocking and blanketing towards realistic models for expanding atmospheres
DOI: 10.1051/0004-6361:20010805 Bibcode: 2001A&A...375..161P

Pauldrach, A. W. A.; Hoffmann, T. L.; Lennon, M.

Spectral analysis of hot luminous stars requires adequate model atmospheres which take into account the effects of NLTE and radiation driven winds properly. Here we present significant improvements of our approach in constructing detailed atmospheric models and synthetic spectra for hot luminous stars. Moreover, as we regard our solution method in…

2001 Astronomy and Astrophysics
IUE 453
EXPORT: Spectral classification and projected rotational velocities of Vega-type and pre-main sequence stars
DOI: 10.1051/0004-6361:20011098 Bibcode: 2001A&A...378..116M

Rauer, H.; Schneider, J.; Eiroa, C. +19 more

In this paper we present the first comprehensive results extracted from the spectroscopic campaigns carried out by the EXPORT (EXoPlanetary Observational Research Team) consortium. During 1998-1999, EXPORT carried out an intensive observational effort in the framework of the origin and evolution of protoplanetary systems in order to obtain clues o…

2001 Astronomy and Astrophysics
IUE 228
High resolution X-ray spectroscopy of zeta Puppis with the XMM-Newton reflection grating spectrometer
DOI: 10.1051/0004-6361:20000093 Bibcode: 2001A&A...365L.312K

Mewe, R.; Güdel, M.; Leutenegger, M. A. +5 more

We present the first high resolution X-ray spectrum of the bright O4Ief supergiant star zeta Puppis, obtained with the Reflection Grating Spectrometer on-board XMM-Newton. The spectrum exhibits bright emission lines of hydrogen-like and helium-like ions of nitrogen, oxygen, neon, magnesium, and silicon, as well as neon-like ions of iron. The lines…

2001 Astronomy and Astrophysics
IUE XMM-Newton 182
The mass of the neutron star in Vela X-1
DOI: 10.1051/0004-6361:20011122 Bibcode: 2001A&A...377..925B

Kaper, L.; Telting, J. H.; Barziv, O. +2 more

We measured the radial-velocity curve of HD 77581, the B-supergiant companion of the X-ray pulsar Vela X-1, using 183 high-resolution optical spectra obtained in a nine-month campaign. We derive radial-velocity amplitudes for different lines and wavelength regions, and find all are consistent with each other, as well as with values found in previo…

2001 Astronomy and Astrophysics
IUE 164
The ISO-SWS spectrum of planetary nebula NGC 7027
DOI: 10.1051/0004-6361:20000435 Bibcode: 2001A&A...367..949B

Pottasch, S. R.; Beintema, D. A.; Bernard Salas, J. +1 more

We present the infrared spectrum of the planetary nebula NGC 7027 observed with the Short Wavelength Spectrometer (SWS), on board the Infrared Space Observatory (ISO). These data allow us to derive the electron density and, together with the IUE and optical spectra, the electron temperature for several ions. The nebular composit…

2001 Astronomy and Astrophysics
ISO IUE 103
Time-resolved spectral analysis of the pulsating helium star V652 Her
DOI: 10.1051/0004-6361:20010954 Bibcode: 2001A&A...376..497J

Jeffery, C. S.; Woolf, V. M.; Pollacco, D. L.

A series of 59 moderate-resolution high signal-to-noise spectra of the pulsating helium star V652 Her covering 1.06 pulsation cycles was obtained with the William Herschel Telescope. These have been supplemented by archival ultraviolet and visual spectrophotometry and used to make a time-dependent study of the properties of

2001 Astronomy and Astrophysics
IUE 97
Helium-like triplet density diagnostics. Applications to CHANDRA-LETGS X-ray observations of Capella and Procyon
DOI: 10.1051/0004-6361:20000419 Bibcode: 2001A&A...367..282N

Schmitt, J. H. M. M.; Kaastra, J. S.; Burwitz, V. +6 more

Electron density diagnostics based on the triplets of helium-like C v, N vi, and O vii are applied to the X-ray spectra of Capella and Procyon measured with the Low Energy Transmission Grating Spectrometer (LETGS) on board the Chandra X-ray Observatory. New theoretical models for the calculation of the line ratios between the forbidden (f), interc…

2001 Astronomy and Astrophysics
IUE 92
Non-axisymmetric accretion on the classical TTS RW Aur A
DOI: 10.1051/0004-6361:20010203 Bibcode: 2001A&A...369..993P

Tuominen, I.; Gahm, G. F.; Gameiro, J. F. +5 more

High-resolution spectroscopic monitoring of the exceptionally active classical T Tauri star (CTTS) RW Aur A was carried out in three seasons of 1996, 1998 and 1999 with simultaneous B, V photometry. The high quality spectra revealed a multicomponent structure of the spectrum, which includes: 1) a veiled photospheric spectrum of a K1-K4 star, 2) br…

2001 Astronomy and Astrophysics
IUE 91
A search for the cause of cyclical wind variability in O stars. Simultaneous UV and optical observations including magnetic field measurements of the O7.5III star xi Persei
DOI: 10.1051/0004-6361:20000570 Bibcode: 2001A&A...368..601D

Kaper, L.; Bohlender, D. A.; Gordon, K. +13 more

We present the results of an extensive observing campaign on the O7.5 III star xi Persei. The UV observations were obtained with the International Ultraviolet Explorer. xi Per was monitored continuously in October 1994 during 10 days at ultraviolet and visual wavelengths. The ground-based optical observations …

2001 Astronomy and Astrophysics
IUE 66
The INES system. IV. The IUE absolute flux scale
DOI: 10.1051/0004-6361:20010646 Bibcode: 2001A&A...373..730G

Wamsteker, W.; González-Riestra, R.; Cassatella, A

This paper deals with the definition of the input fluxes used for the calibration of the IUE Final Archive. The method adopted consists in the determination of the shape of the detector's sensitivity curves using IUE low resolution observations with model fluxes of the DA white dwarf G191-B2B. A scale factor was then determined so that the IUE obs…

2001 Astronomy and Astrophysics
IUE eHST 49