Search Publications

The Ulysses mission.
Bibcode: 1998SciAm.278a..52S

Smith, E. J.; Marsden, R. G.

Of the dozens of spacecraft sent to explore the solar system, only Ulysses has veered far from the ecliptic. Now looping over the sun's poles in an orbit as wide as Jupiter's, Ulysses has a unique view of the solar wind that is advancing stellar astrophysics.

1998 Scientific American
Ulysses 0
Quasi-periodic oscillations in celestial X-ray sources
DOI: 10.1038/scientificamerican1188-50 Bibcode: 1988SciAm.259e..50V

van der Klis, Michiel

Exosat observations of the X-ray sources and the discovery of QPOs of GX5-1 are discussed. Recent developments in X-ray astronomy are reviewed. Also, possible models to explain QPOs in X-ray sources are examined.

1988 Scientific American
Exosat 0
A superluminous object in the Large Cloud of Magellan
DOI: 10.1038/scientificamerican0884-52 Bibcode: 1984SciAm.251b..52M

Savage, B. D.; Cassinelli, J. P.; Mathis, J. S.

The superluminous object R136a of the nebula 30 Dor in the Large Cloud of Magellan is characterized, summarizing the results of recent optical and (IUE) UV observations. Photographs, spectra, and diagrams are provided; and the techniques used to determine the parameters of the object are explained. The UV spectra exhibit a typical P Cygni profile …

1984 Scientific American
IUE 1
Epsilon Aurigae
DOI: 10.1038/scientificamerican1084-98 Bibcode: 1984SciAm.251d..98H

Hack, M.

The results of recent ultraviolet and deep infrared observations of the latest eclipse of the binary Epsilon Aurigae are reported. The observations were performed with both the International Ultraviolet Explorer (IUE) satellite, and with the three-meter Infrared Telescope at Mauna Kea, Hawaii. On the basis of new theoretical models, several explan…

1984 Scientific American
IUE 1
The coronas of galaxies
DOI: 10.1038/scientificamerican0882-54 Bibcode: 1982SciAm.247b..54D

Savage, B. D.; de Boer, K. S.

The instrumentation and results of observations of interstellar and intergalactic gases are reviewed, particularly for UV satellite data on the dynamics and composition of the galactic corona. Radio telescopes began the mapping of gas in the central galactic disk in the 1950's, using 21-cm readings to detect atomic hydrogen clouds 100,000 light ye…

1982 Scientific American
IUE 0