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An investigation of the B335 region through far infrared spectroscopy with ISO
Bibcode: 1999A&A...343..266N

Liseau, R.; White, G. J.; Benedettini, M. +11 more

We present far infrared spectra of the B335 dark cloud region, obtained with the Long Wavelength Spectrometer (LWS) on-board the ISO satellite. Deep spectra were obtained towards the far infrared outflow exciting source, located in the B335 core, and on the three associated Herbig Haro (HH) objects HH119 A, B and C. In addition, a region of about …

1999 Astronomy and Astrophysics
ISO 22
A non-local thermodynamic equilibrium spherical line-blanketed stellar atmosphere model of the early B giant beta CMa
DOI: 10.1046/j.1365-8711.1999.02140.x Bibcode: 1999MNRAS.302..599A

Hauschildt, P. H.; Baron, E.; Aufdenberg, J. P.

The observed multiwavelength spectrum of the B1II--III star beta CMa is successfully reproduced, including the extreme ultraviolet (EUV) continuum observed by Extreme Ultraviolet Explorer (EUVE), with a non-local thermodynamic equilibrium fully line-blanketed spherical hydrostatic model atmosphere. The available spectrophotometry of beta CMa from …

1999 Monthly Notices of the Royal Astronomical Society
Hipparcos IUE 22
Chromospheric imaging of the active binary system V 711 Tauri = HR 1099 in December 1992
Bibcode: 1999A&A...350..571B

Pagano, I.; Lanzafame, A. C.; Rodonò, M. +2 more

Spectroscopic observations of the bright RS CVn-type system V 711 Tau = HR 1099 (K1 IV + G5 V) were obtained by IUE during the same period of a Multi-Site Continuous Spectroscopy (MUSICOS) campaign between 12-18 December 1992 (Huang et al. 1995). We report on the results of a ``Doppler Imaging" analysis of the Mg II h line. Broad, variable and ext…

1999 Astronomy and Astrophysics
IUE 22
Ultraviolet and Optical Line Profile Variations in the Spectrum of ɛ Persei
DOI: 10.1086/307872 Bibcode: 1999ApJ...525..420G

Kambe, E.; Gies, D. R.; Riddle, R. L. +13 more

The rapid variable star, ɛ Per (B0.5 IV-III), displays the largest amplitude profile fluctuations known among the growing number of massive, spectrum-variable stars. Here we present an analysis of a continuous 5 day run of IUE UV spectroscopy, and we show for the first time that the systematic, blue-to-red moving patterns observed in high-quality …

1999 The Astrophysical Journal
IUE 22
Lines of OIV and SIV in the Goddard High-Resolution Spectrograph spectrum of RR Tel: constraints on atomic data
DOI: 10.1046/j.1365-8711.1999.02392.x Bibcode: 1999MNRAS.303L..41H

Judge, P. G.; Carpenter, K. G.; Jordan, C. +3 more

High signal-to-noise ratio spectra of RR Tel obtained at medium resolution with the Goddard High-Resolution Spectrograph (GHRS) on the Hubble Space Telescope (HST) are used to test available atomic data for the OIV 2s^22p ^2P-2s2p^2 ^4P multiplet (UV 0.01). The fine-structure intervals of the 2s2p^2 ^4P term given by Moore (1983) appear to need re…

1999 Monthly Notices of the Royal Astronomical Society
eHST 22
Total solar irradiance variations
DOI: 10.1016/S1364-6826(98)00112-6 Bibcode: 1999JASTP..61...15P

Fröhlich, C.; Pap, J. M.

Total solar irradiance has been monitored from space for nearly two decades. These space-borne observations have established conclusively that total solar irradiance changes over a wide range of periodicities-from minutes to the 11-year solar cycle. Since the total energy flux of the Sun is the principal driver for all Earths atmospheric phenomena…

1999 Journal of Atmospheric and Solar-Terrestrial Physics
SOHO 22
SN 1994D in NGC 4526: a normally bright type IA supernova
DOI: 10.48550/arXiv.astro-ph/9907345 Bibcode: 1999A&A...349..877D

Richtler, Tom; Drenkhahn, Georg

SN 1994D of type Ia has been suspected not to fit into the relation between decline rate, colour, and brightness. However, an individual distance of its host galaxy, NGC 4526, other than that of the Virgo cluster, has not yet been published. We determined the distance by the method of globular cluster luminosi…

1999 Astronomy and Astrophysics
eHST 22
Application of Realistic Model Atmospheres to Eclipse Maps of Accretion Disks: The Effective Temperature and Flare of the Disk in the Dwarf Nova Z Chamaeleontis
DOI: 10.1086/306974 Bibcode: 1999ApJ...514..952R

Wood, Janet H.; Wade, Richard A.; Robinson, Edward L.

In a previous paper we presented ultraviolet (λeff=1550 Å) high-speed photometry of the eclipsing dwarf nova Z Cha obtained near the peak of a normal eruption, and we derived a maximum-entropy disk map from the eclipse light curve. In the present paper we report a new calculation of the disk map and temperature profile. The calculation …

1999 The Astrophysical Journal
eHST 22
Consistency of accretion discs with Seyfert 1 UV fluxes and Hβ emission-line profiles
DOI: 10.1046/j.1365-8711.1999.02565.x Bibcode: 1999MNRAS.307...41R

Boisson, C.; Rokaki, E.

This paper presents accretion disc fits to the UV continuum and Hβ emission line in a complete sample of broad-emission-line AGN sources. Disc fits to the UV continuum emission leave an ambiguity between the central mass and the orientation of the disc in that more massive black holes mimic more edge-on discs. The opposite dependence between mass …

1999 Monthly Notices of the Royal Astronomical Society
IUE 22
Accurate Optical Positions of Extragalactic Radio Reference Frame Sources
DOI: 10.1086/301083 Bibcode: 1999AJ....118.2511Z

Zacharias, N.; Zacharias, M. I.; Hall, D. M. +3 more

Optical positions on the 50 mas level in the Hipparcos system have been obtained for 327 extragalactic, radio reference frame sources for both hemispheres from a 2-step procedure. Positions of secondary reference stars in the 10<=V<=14 magnitude range were obtained from photographic plates taken at the Hamburg astrograph (Northern Hemisphere…

1999 The Astronomical Journal
Hipparcos 22