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Globular Clusters Photometry With the Hubble Space Telescope. III. Blue Stragglers and Variable Stars in the Core of M3
DOI: 10.1086/117193 Bibcode: 1994AJ....108.1786G

Schneider, D. P.; Yanny, B.; Guhathakurta, P. +1 more

This paper describes Hubble Space Telescope (HST)/Planetary Camera-I images of the core of the dense globular cluster M3 (NGC 5272). Stellar photometry in the F555W (V) and F785LP (I) bands, with a 1-sigma photometric accuracy of about 0.1 mag, has been used to construct color-magnitude diagrams of about 4700 stars above the main-sequence turnoff …

1994 The Astronomical Journal
eHST 35
Multi-site continuous spectroscopy. II. Spectrophotometry and energy budget of exceptional white-light flares on HR1099 from the MUSICOS 89 campaign.
Bibcode: 1994A&A...292..543F

Zhang, X.; de La Reza, R.; Keskin, V. +48 more

We report results from the December 89 multi-site continuous observing campaign (MUSICOS 89) dedicated to the study of surface active structures and flares on the RS CVn-type system HR1099 (=V711 Tau). This system has been observed by up to 17 telescopes around the globe during this campaign. We obtained complete phase coverage for Doppler imaging…

1994 Astronomy and Astrophysics
IUE 35
Remarkable Long-Term Changes in the Small Magellanic Cloud Wolf-Rayet System HD 5980
DOI: 10.1086/174905 Bibcode: 1994ApJ...436..301K

Koenigsberger, G.; Auer, L. H.; Moffat, A. F. J. +3 more

In this paper we report the remarkable changes which occurred in the Small Magellanic Cloud W-R system HD5980 = AB5 between 1978 and 1991. Within this timescale, there has been a systematic enhancement (by factors of 2-10 depending on the line) in the equivalent widths of all emission lines, and a change in the relative strengths of N III, N IV, a…

1994 The Astrophysical Journal
IUE 35
Eclipse Mapping of the Accreting Magnetic White Dwarf in DP Leonis with HST
DOI: 10.1086/174407 Bibcode: 1994ApJ...430..323S

Holberg, J. B.; Liebert, James; Schmidt, Gary D. +1 more

We present time-resolved ultraviolet spectrophotometry of the AM Her system DP Leo (E1114+182), obtained with the Faint Object Spectrograph on the Hubble Space Telescope (HST) in 1991 October. During this period, the binary was in a low-activity state. Complementary optical spectrophotometry and spectopolarimetry were obtained in 1991 October and …

1994 The Astrophysical Journal
eHST 35
The IMF and the extinction law in M 101: HST FOS spectra of extragalactic HII regions.
Bibcode: 1994A&A...291....1R

Benvenuti, P.; Rosa, M. R.

We present medium resolution HST FOS spectra of the ionizing star clusters in four giant HII regions in the spiral galaxy M101, spanning a range in [O/H] from 8.2 to 8.9. The observed energy distributions in the wavelength range 1150A to 8200A are compared to population synthesis models of extremely young star clusters, taking into account the att…

1994 Astronomy and Astrophysics
eHST 35
Interplanetary type III radio bursts that approach the plasma frequency: ULYSSES observations.
Bibcode: 1994A&A...289..957H

Hoang, S.; Leblanc, Y.; Dulk, G. A.

We study a set of solar type III radio bursts where the emission is visible from the high-frequency limit of the radio astronomy receiver of the Ulysses Unified Radio and Plasma wave (URAP) experiment down to low frequencies, sometimes near the plasma frequency, and where Langmuir wave spikes are recorded by the radio and/or plasma receivers. For …

1994 Astronomy and Astrophysics
Ulysses 35
Ultraviolet Interstellar Polarization Observed with the Hubble Space Telescope
DOI: 10.1086/187361 Bibcode: 1994ApJ...427L..47S

Martin, P. G.; Walsh, J. R.; Nandy, K. +9 more

We have used the Faint Object Spectrograph of the Hubble Space Telescope to observe interstellar linear polarization from 1300 to 3300 A in two stars with well-studied interstellar polarization at visible wavelenths. The wavelength dependence of linear polarization declines smoothly with decreasing wavelength and is devoid of structure associated …

1994 The Astrophysical Journal
eHST 35
HST observations of globular clusters in M 31 I. Surface photometry of 13 objects.
DOI: 10.48550/arXiv.astro-ph/9310030 Bibcode: 1994A&A...284..349F

Cacciari, C.; Federici, L.; Ferraro, F. R. +8 more

We present the initial results of a study of globular clusters in M 31, using the Faint Object Camera (FOC) on the Hubble Space Telescope (HST). The sample of objects consists of 13 clusters spanning a range of properties. Three independent image deconvolution techniques were used in order to compensate for the optical problems of the HST, leading…

1994 Astronomy and Astrophysics
eHST 35
Disk-Resolved Imaging of Io with the Hubble Space Telescope
DOI: 10.1006/icar.1994.1062 Bibcode: 1994Icar..108..272S

McGrath, Melissa A.; Paresce, Francesco; Sartoretti, Paola

The first disk-resolved image of Io's trailing hemisphere in the ultraviolet, as well as a visible image of the same hemisphere, has been obtained with the Faint Object Camera (FOC) of the Hubble Space Telescope on March 15, 1992, at a resolution of 210 km. Io shows no large-scale changes in the visible over the 13 years elapsed since the last dis…

1994 Icarus
eHST 35
Solar and Heliospheric Processes from Solar Wind Composition Measurements
DOI: 10.1098/rsta.1994.0126 Bibcode: 1994RSPTA.349..213G

Geiss, J.; Gloeckler, G.; von Steiger, R.

Composition measurements in the solar wind provide important information for solar system science and astrophysics. We show in this report how ion composition data are used to investigate chromospheric and coronal processes. Isotopic abundances in the Sun can best be derived from solar wind measurements. 3He/4He is an isotopi…

1994 Philosophical Transactions of the Royal Society of London Series A
Ulysses 34