Search Publications

Infrared Space Observatory Measurements of [C II] Line Variations in Galaxies
DOI: 10.1086/311044 Bibcode: 1997ApJ...491L..27M

Helou, G.; Stacey, G.; Malhotra, S. +11 more

We report measurements of the [C II] fine-structure line at 157.714 µm in 30 normal star-forming galaxies with the Long Wavelength Spectrometer (LWS) on the Infrared Space Observatory (ISO). The ratio of the line to total far-infrared (FIR) luminosity, L[CII]/LFIR, measures the ratio of the cooling of gas to that of dus…

1997 The Astrophysical Journal
ISO 196
On the Evolutionary Phase and Mass Loss of the Wolf-Rayet--like Stars in R136a
DOI: 10.1086/303736 Bibcode: 1997ApJ...477..792D

Hubeny, Ivan; Heap, Sara R.; de Koter, Alex

We report on a systematic study of the most massive stars, in which we analyzed the spectra of four very luminous stars in the Large Magellanic Cloud. The stars lie in the 30 Doradus complex, three of which are located in the core of the compact cluster, R136a (R136a1, R136a3, and R136a5), and the fourth (Melnick 42), located about 8" north of R13…

1997 The Astrophysical Journal
eHST 195
Geologic Mapping of Vesta from 1994 Hubble Space Telescope Images
DOI: 10.1006/icar.1997.5734 Bibcode: 1997Icar..128...95B

Wells, Eddie N.; Storrs, Alex D.; Thomas, Peter C. +3 more

We utilize the 56 images of Asteroid 4 Vesta obtained through four mineralogically diagnostic filters by the Hubble Space Telescope (Zellneret al.1997,Icarus) to construct a geologic map. Vesta's surface is found to be geologically diverse and to be dichotomous at a hemispheric scale. The eastern hemisphere (longitude definition from Thomaset al.1…

1997 Icarus
eHST 194
SN IA light curves and radioactive decay
DOI: 10.48550/arXiv.astro-ph/9707016 Bibcode: 1997A&A...328..203C

Turatto, M.; Cappellaro, E.; Benetti, S. +4 more

The absolute V light curves of 5 SNe Ia, selected to represent the known range of absolute luminosities at maximum for this class of objects, are presented. Comparison of the long term luminosity evolution shows that the differences seen at maximum persist, and actually increase with time, reinforcing the notion that intrinsic differences do exist…

1997 Astronomy and Astrophysics
eHST 194
EIT and LASCO Observations of the Initiation of a Coronal Mass Ejection
DOI: 10.1023/A:1004907307376 Bibcode: 1997SoPh..175..601D

Llebaria, A.; St. Cyr, O. C.; Michels, D. J. +31 more

We present the first observations of the initiation of a coronal mass ejection (CME) seen on the disk of the Sun. Observations with the EIT experiment on SOHO show that the CME began in a small volume and was initially associated with slow motions of prominence material and a small brightening at one end of the prominence. Shortly afterward, the p…

1997 Solar Physics
SOHO 193
Steps toward Determination of the Size and Structure of the Broad-Line Region in Active Galactic Nuclei. IX. Ultraviolet Observations of Fairall 9
DOI: 10.1086/312996 Bibcode: 1997ApJS..110....9R

Shull, J. M.; Malkan, M. A.; Martin, P. G. +53 more

An 8 month monitoring campaign on the Seyfert 1 galaxy Fairall 9 has been conducted with the International Ultraviolet Explorer in an attempt to obtain reliable estimates of continuum-continuum and continuum-emission-line delays for a high-luminosity active galactic nucleus (AGN). While the results of this campaign are more ambiguous than those of…

1997 The Astrophysical Journal Supplement Series
IUE 192
Polar Plume Anatomy: Results of a Coordinated Observation
DOI: 10.1023/A:1004955223306 Bibcode: 1997SoPh..175..393D

Plunkett, S. P.; Thompson, B. J.; Gurman, J. B. +5 more

On 7 and 8 March 1996, the SOHO spacecraft and several other space- and ground-based observatories cooperated in the most comprehensive observation to date of solar polar plumes. Based on simultaneous data from five instruments, we describe the morphology of the plumes observed over the south pole of the Sun during the SOHO observing campaign. Ind…

1997 Solar Physics
SOHO 190
Time-Distance Helioseismology with the MDI Instrument: Initial Results
DOI: 10.1023/A:1004907220393 Bibcode: 1997SoPh..170...63D

Kosovichev, A. G.; Hoeksema, J. T.; Scherrer, P. H. +10 more

In time-distance helioseismology, the travel time of acoustic waves is measured between various points on the solar surface. To some approximation, the waves can be considered to follow ray paths that depend only on a mean solar model, with the curvature of the ray paths being caused by the increasing sound speed with depth below the surface. The …

1997 Solar Physics
SOHO 188
Microvariability survey with the Hubble Space Telescope Fine Guidance Sensors. Exploring the instrumental properties
Bibcode: 1997A&A...328..544K

Kuschnig, R.; Weiss, W. W.; Gruber, R. +2 more

The suitability of the Hubble Space Telescope (HST) Fine Guidance Sensors (FGS) for a magnitude limited survey of microvariability among guide stars is investigated. The linearity, relative sensitivity, and dead-time constants of the three FGSs are determined, and the photon noise limitation of the FGS photometry is confirmed. The noise spectrum i…

1997 Astronomy and Astrophysics
eHST 186
Infrared spectroscopy of interstellar apolar ice analogs
Bibcode: 1997A&A...328..649E

van Dishoeck, E. F.; Tielens, A. G. G. M.; Boogert, A. C. A. +2 more

Apolar ices have been observed in several regions in dense clouds and are likely dominated by molecules such as CO, CO_2 and the infrared inactive molecules O_2 and N_2. Interstellar solid CO has been well characterized by ground-based high resolution measurements. Recent ISO results showed the ubiquitous presence of abundant CO_2 ice and the pres…

1997 Astronomy and Astrophysics
ISO 185