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Ultraviolet and Optical Spectral Morphology of Melnick 42 and Radcliffe 136a in 30 Doradus
DOI: 10.1086/186439 Bibcode: 1992ApJ...393L..13W

Walborn, Nolan R.; Ebbets, Dennis C.; Parker, Joel Wm. +2 more

HST/GHRS ultraviolet spectrograms of the individual O3 If */WN6-A object Mk 42 in 30 Dor and the adjacent, central multiple system R136a are compared with each other and with an appropriate sequence of O3 If* and WN6-A standards from the IUE archive. The analogous spectral montages covering the blue-violet region, based on new, homogeneous, digita…

1992 The Astrophysical Journal
IUE eHST 32
Ulysses plasma observations of coronal mass ejections near 2.5 AU
DOI: 10.1029/92GL00529 Bibcode: 1992GeoRL..19.1239P

Balogh, A.; McComas, D. J.; Forsyth, R. J. +5 more

The Ulysses solar wind plasma experiment observed a series of interplanetary shocks and coronal mass ejections (CMEs), the latter evidenced by counterstreaming electrons and a variety of ion signatures, during March and April 1991. A striking sequence was observed near 2.5 AU from March 23 through April 2, with the second of two counterstreaming e…

1992 Geophysical Research Letters
Ulysses 32
Stratification of chemical elements in the atmosphere of the AP star 53 Camelopardalis.
Bibcode: 1992A&A...263..232B

Babel, J.; Lanz, T.

A detailed abundance analysis of Cr, Fe, Mn, Ca, and Ti in the Ap star 53 Cam from IUE high-resolution spectra has been performed. It is found that UV lines give significantly lower abundance than visible lines for Cr and Fe. Theoretical spectra of Cr II line calculated with the stratified chromium abundance distributions predicted a priori by the…

1992 Astronomy and Astrophysics
IUE 32
The outer atmospheres of the 'hybrid' bright giants : the chromospheres of alpha TrA (K4 II), IOTA AUR (K3 II), gamma AQL (K3 II) , and theta HER (K1 II).
DOI: 10.1093/mnras/256.1.37 Bibcode: 1992MNRAS.256...37H

Harper, Graham M.

Detailed models of the chromospheres of several 'hybrid' bright giants are presented. The models extend from the base of the chromosphere and into the transition area. These chromospheric models are based on radiative transfer calculations for a range of atoms and emission lines. The presence of steep turbulent velocity gradients leads to profiles…

1992 Monthly Notices of the Royal Astronomical Society
IUE 32
Far-Ultraviolet Observations of the Crab Nebula Using the Hopkins Ultraviolet Telescope
DOI: 10.1086/171952 Bibcode: 1992ApJ...399..611B

Blair, William P.; Kriss, Gerard A.; Davidsen, Arthur F. +5 more

Observations of the FUV spectrum of the central portion of the Crab Nebula SNR using the Hopkins Ultraviolet Telescope (HUT) aboard the Astro-1 space shuttle mission in December 1990 are reported. The C IV 1549-A emission line shows two resolved components representing the front and back sides of the shell expanding at roughly +/- 1100 km/s. The H…

1992 The Astrophysical Journal
IUE 31
R Aquarii : an attempt at a unified model.
Bibcode: 1992A&A...262...83B

Burgarella, D.; Vogel, M.; Paresce, F.

Consideration is given to a new model of R Aqr in which the binary system is composed of an M7 Mira with a mass of about 1.5 solar mass, a temperature of about 2800 K, a bolometric magnitude of about -4.56, and a radius of about 300 solar radii, plus a hot stellar source in an intermediate phase between a subdwarf and a white dwarf with a radiatio…

1992 Astronomy and Astrophysics
eHST 31
Time dependence of the UV resonance lines in the cataclyspic variables YZCnc, IR GEM and V 3885 Sgr.
DOI: 10.1093/mnras/255.2.237 Bibcode: 1992MNRAS.255..237W

Verbunt, F.; Collier Cameron, A.; Woods, J. A. +2 more

Orbital variations are observed in the UV resonance lines of YZ Cnc, IR Gem and V3885 Sgr. Optical spectroscopic observations of YZ Cnc show that the maximum absorption in the UV lines occurs about 0.7-0.8 orbits after the transition from red to blue of the optical emission lines. IR Gem shows orbital variations in the UV lines that are as strong …

1992 Monthly Notices of the Royal Astronomical Society
IUE 31
Hubble space telescope observations of the 1990 equatorial disturbance on Saturn: Images, albedos, and limb darkening
DOI: 10.1016/0019-1035(92)90112-K Bibcode: 1992Icar..100..485W

Ingersoll, Andrew P.; Baum, William A.; Westphal, James A. +4 more

In September 1990 a major equatorial eruption on Saturn produced a disturbance that spread in longitude until it completely girdled the planet. We report here on 150 images recorded in six passbands with the Wide Field/Planetary Camera (WF/PC) aboard the Hubble Space Telescope (HST) on 17 and 18 November 1990. For comparison, we used HST-WF/PC obs…

1992 Icarus
eHST 31
Hubble Space Telescope Imaging of the Large-Redshift Gravitational Lens Candidate 1208+1011
DOI: 10.1086/186411 Bibcode: 1992ApJ...392L...1B

Maoz, Dan; Schneider, Donald P.; Yanny, Brian +2 more

Four-color photometry obtained with the Hubble Space Telescope is consistent with the hypothesis that the light from the quasar 1208+1011 (z = 3.8) is gravitationally lensed. Guided exposures taken with the HST Planetary Camera resolve the quasar image into two point-source components separated by 0.476" +/- 0.004". The intensity ratio of the comp…

1992 The Astrophysical Journal
eHST 30
A Gravitational Lens Candidate Discovered with the Hubble Space Telescope
DOI: 10.1086/186278 Bibcode: 1992ApJ...386L...1M

Filippenko, Alexei V.; Maoz, Dan; Schneider, Donald P. +6 more

We report evidence for gravitational lensing of the high-redshift (z = 3.8) quasar 1208+101, observed as part of the Snapshot Survey with the Hubble Space Telescope Planetary Camera. An HST V image taken on gyroscopes resolves the quasar into three point-source components, with the two fainter images having separations of 0.1" and 0.5" from the ce…

1992 The Astrophysical Journal
eHST 30