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Iron and nickel abundances of subluminous O-stars. I. NLTE-model atmospheres with line blanketing by iron group elements.
Bibcode: 1996A&A...311..669H

Werner, K.; Dreizler, S.; Heber, U. +2 more

NLTE model atmospheres for hot evolved stars including line blanketing of all iron group elements were first constructed by Dreizler & Werner (1993). In this paper we improve computational details and check the adopted simplifications. We also present a systematic investigation of the consequences of iron group line blanketing on the atmospher…

1996 Astronomy and Astrophysics
IUE 33
The Environments of Supernovae in Archival Hubble Space Telescope Images
DOI: 10.1086/117940 Bibcode: 1996AJ....111.2047B

Filippenko, Alexei V.; Leibundgut, Bruno; Barth, Aaron J. +2 more

We have examined the immediate environments of several supernovae using archival prerefurbishment Hubble Space Telescope images to search for clues to the nature of the progenitor stars. For the Type II supernova 1968L in M83 the colors of nearby star clusters indicate ages of <~ 6-7 x 10^6^ yr, implying an initial mass of ~> 25-30 M_sun_ fo…

1996 The Astronomical Journal
eHST 33
The mid-infrared color of NGC 6946.
DOI: 10.48550/arXiv.astro-ph/9610241 Bibcode: 1996A&A...315L.157H

Helou, G.; Lord, S. D.; Malhotra, S. +10 more

We analyze the new mid-infrared maps of NGC 6946 for variations in the color ratio of the 7-to-15µm emission. Our preliminary findings are that this mid-infrared color is remarkably constant between arms and inter-arm regions, and as a function of radius in the disk, excluding the nuclear region. As surface brightness ranges by more than an …

1996 Astronomy and Astrophysics
ISO 32
A Candidate Gravitational Lens in the Hubble Deep Field
DOI: 10.1086/310213 Bibcode: 1996ApJ...467L..73H

Hogg, David W.; Fassnacht, C. D.; Blandford, Roger +2 more

The discovery of HDF J123652+621227, a candidate gravitational lens in the Hubble Deep Field, is reported. This lens may be multiply imaging several optical sources at different redshifts. If follow-up spectroscopy of the lens and the brightest image confirms this hypothesis, observations of this system alone can be used to obtain an estimate of t…

1996 The Astrophysical Journal
eHST 32
Spectroscopy of Bright Quasars with the Hubble Space Telescope and Lyman-Alpha Absorption Lines in the Redshift Range 0.5 < Z < 1.7
DOI: 10.1086/177262 Bibcode: 1996ApJ...463..473I

Malkan, M. A.; Impey, C. D.; Petry, C. E. +1 more

We report ultraviolet spectroscopy of three bright quasars obtained with the Faint Object Spectrograph of the Hubble Space Telescope. The good quality spectra covering the range 1800-3300 A result from spectropolarimetry acquired for these targets, the interpretation of which has been published elsewhere. Objective algorithms were used to select a…

1996 The Astrophysical Journal
eHST 32
Theoretical amplitudes of solar g-modes.
Bibcode: 1996A&A...312..610A

Andersen, B. N.

This work presents predictions on the amplitudes of solar g-modes. It is based on the assumption that convective overshoot into the convectively stable interior generates gravity waves. Based on this assumption it is possible to estimate values for the amplitude of the g-modes below the solar convection zone. Numerical simulations, giving the tran…

1996 Astronomy and Astrophysics
SOHO 32
Hubble Space Telescope Observations of the Seyfert Galaxy NGC 3783: Discovery of Variable C IV Absorption
DOI: 10.1086/177457 Bibcode: 1996ApJ...465..733M

Hutchings, John B.; Reichert, Gail A.; Mushotzky, Richard F. +5 more

We have discovered variable absorption lines in HST spectra of the Seyfert 1 galaxy NGC 3783. C IV λλ1548.2, 1550.8 absorption is present in an FOS spectrum on 1992 July 27 and a GHRS spectrum on 1994 January 16 at a radial velocity of -450 km s^-1^ relative to the emission-line peak, but there is no evidence for absorption in a GHRS spectrum on 1…

1996 The Astrophysical Journal
eHST 32
The regular structure of shock-accelerated ~40-100keV electrons in the high latitude heliosphere.
Bibcode: 1996A&A...316..481R

Simnett, G. M.; Tappin, S. J.; Roelof, E. C.

The passage of Ulysses through the high latitude heliosphere has given us a new insight into the interplanetary dynamical processes which are occurring, at any rate near solar minimum, in the heliosphere above the streamer belt. We report here observations of ~40-100keV electrons and ~0.5MeV protons detected by HI-SCALE from 1992-96. Apart from a …

1996 Astronomy and Astrophysics
Ulysses 32
Hubble Space Telescope/FOS Spectroscopy of VW Hydri in Superoutburst
DOI: 10.1086/176818 Bibcode: 1996ApJ...458..355H

Szkody, P.; Sion, E. M.; Huang, M. +2 more

We present an analysis of two HST/FOS UV spectra of the SU UMa type dwarf nova, VW Hyi, obtained on 1993 October 24, ∼5 days after the optical rise of a superoutburst The absorption features in the first spectrum appear to consist of two components: a broad-winged component (with velocity width of 3000 km s-1) and a sharp core narrow co…

1996 The Astrophysical Journal
eHST 32
The Masses and Radii of the Eclipsing Binary zeta Aurigae
DOI: 10.1086/177981 Bibcode: 1996ApJ...471..454B

Harper, Graham M.; Bennett, Philip D.; Brown, Alexander +1 more

We present a full determination of the fundamental stellar and orbital parameters of the eclipsing binary ζ Aurigae (K4 Ib + BS V) using recent observations with the Hubble Space Telescope Goddard High Resolution Spectrograph (GHRS) and the Mark III long-baseline optical interferometer. The information obtained from spectroscopic and interferometr…

1996 The Astrophysical Journal
eHST 31