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The Early Ultraviolet Spectral Evolution of Nova Cygni 1992
DOI: 10.1086/116812 Bibcode: 1993AJ....106.2408S

Ake, T. B.; Shore, Steven N.; Sonneborn, George +2 more

We report on the high resolution ultraviolet line profile evolution of Nova Cygni 1992 using the International Ultraviolet Explorer (IUE) satellite and the Goddard High Resolution Spectrograph (GHRS) on the Hubble Space Telescope (HST). Our observations cover the period from discovery in 1992 February through 1993 April. The initial expansion velo…

1993 The Astronomical Journal
IUE eHST 83
Synthetic UV Lines of Si IV, C IV, and He II from a Population of Massive Stars in Starburst Galaxies
DOI: 10.1086/173432 Bibcode: 1993ApJ...418..749R

Robert, Carmelle; Heckman, Timothy M.; Leitherer, Claus

We present the first results of our study of the massive star population in starburst galaxies based on UV data. We have synthesized the Si IV 1400, C IV 1550 and He II 1640 lines for both a continuous and an instantaneous burst of star formation with approximately solar chemical composition. Our code uses the latest generation of stellar evolutio…

1993 The Astrophysical Journal
IUE 81
A model for the 89 Herculis system.
Bibcode: 1993A&A...269..242W

Waters, L. B. F. M.; Mayor, M.; Trams, N. R. +1 more

We report new radial velocity measurements of the F2 supergiant 89 Her that confirm the binary nature of this star. A period search yields an orbital period of 288.4 +/- 0.7 days, in close agreement with earlier results. We also present intermediate resolution spectra in the wavelength range 3500 - 11,000 A, with numerous emission lines. We use th…

1993 Astronomy and Astrophysics
IUE 80
Counterstreaming suprathermal electron events upstream of corotating shocks in the solar wind beyond ∼2 Au: Ulysses
DOI: 10.1029/93GL02489 Bibcode: 1993GeoRL..20.2335G

McComas, D. J.; Goldstein, B. E.; Bame, S. J. +3 more

Enhanced fluxes of suprathermal electrons are commonly observed upstream of corotating forward and reverse shocks in the solar wind at heliocentric distances beyond ∼2 AU by the Los Alamos plasma experiment on Ulysses. The average duration of these events, which are most intense immediately upstream from the shocks and which fade with increasing d…

1993 Geophysical Research Letters
Ulysses 77
Detection of Boron, Cobalt, and Other Weak Interstellar Lines toward zeta Ophiuchi
DOI: 10.1086/186957 Bibcode: 1993ApJ...413L..51F

Lambert, D. L.; Federman, S. R.; Gilliland, R. L. +1 more

Numerous weak lines from interstellar atomic species toward Zeta Ophiuchi were observed with the Goddard High-Resolution Spectrograph. Of particular note are the first interstellar detection of cobalt and the detection of boron in this sight line. These measurements provide estimates for the amount of depletion for the two elements. Boron, a volat…

1993 The Astrophysical Journal
eHST 77
On the relative C,N,O abundances and the evolutionary status of yellow symbiotic stars.
Bibcode: 1993A&A...268..159S

Nussbaumer, H.; Schmid, H. M.

Symbiotic binaries consist of a cool giant and a hot radiation source, which is ionizing the nebula associated with the system. Yellow symbiotic stars can be divided according to their IR colors into s-type (stellar) and d'-type (dust) systems. The s-types are relatively narrow systems, with orbital periods of several hundred days. They contain hi…

1993 Astronomy and Astrophysics
IUE 76
First results from the Giotto magnetometer experiment during the P/Grigg-Skjellerup encounter
Bibcode: 1993A&A...268L...5N

Glassmeier, K. -H.; Neubauer, F. M.; Pohl, M. +9 more

The Giotto magnetic field experiment has provided the first magnetic field data on the interaction between the solar wind and a low gas production comet, P/Grigg-Skjellerup. Waves produced by ion pick-up instabilities have been observed throughout the interaction region with particularly simple waveforms at large distances and a rich phenomenology…

1993 Astronomy and Astrophysics
Giotto 75
Spectrophotometry of Wolf-Rayet Stars. I. Continuum Energy Distributions
DOI: 10.1086/172923 Bibcode: 1993ApJ...412..324M

Massey, Philip; Vacca, William D.; Conti, Peter S. +2 more

All available low-resolution IUE spectra are assembled for Galactic, LMC, and SMC W-R stars and are merged with ground-based optical and NIR spectra in order to collate in a systematic fashion the shapes of these energy distributions over the wavelength range 0.1-1 micron. They can be consistently fitted by a power law of the form F(lambda) is app…

1993 The Astrophysical Journal
IUE 74
Ultraviolet Transitions of Low Condensation Temperature Heavy Elements and New Data for Interstellar Arsenic, Selenium, Tellurium, and Lead
DOI: 10.1086/187066 Bibcode: 1993ApJ...416L..41C

Federman, S. R.; Lambert, David L.; Cardelli, Jason A. +1 more

1993 The Astrophysical Journal
eHST 73
On the Lyman-Alpha Emission of Starburst Galaxies
DOI: 10.1086/173454 Bibcode: 1993ApJ...419....7V

Valls-Gabaud, David

Nearby starburst galaxies have consistently shown anomalous Lyα/Hβ ratios. By reanalyzing the published IUE/optical observations, we show that most starbursts present a normal Lyα emission, consistent with case B recombination theory, provided extinction laws appropriate to their metallicities are used. This implies that extinction is more importa…

1993 The Astrophysical Journal
IUE 72