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CELIAS - Charge, Element and Isotope Analysis System for SOHO
DOI: 10.1007/BF00733436 Bibcode: 1995SoPh..162..441H

Livi, S.; Hsieh, K. C.; Wurz, P. +30 more

The CELIAS experiment on SOHO is designed to measure the mass, ionic charge and energy of the low and high speed solar wind, of suprathermal ions, and of low energy flare particles. Through analysis of the elemental and isotopic abundances, the ionic charge state, and the velocity distributions of ions originating in the solar atmosphere, the inve…

1995 Solar Physics
SOHO 259
WFPC2 Studies of the Crab Nebula. I. HST and ROSAT Imaging of the Synchrotron Nebula
DOI: 10.1086/175956 Bibcode: 1995ApJ...448..240H

Casertano, Stefano; Ballester, Gilda E.; Crisp, David +18 more

We present images of the Crab synchrotron nebula obtained with the Wide Field and Planetary Camera 2 (WFPC2) on board the Hubble Space Telescope. These data are compared with ROSAT HRI images, and with 0."5 resolution Canada-France-Hawaii Telescope (CFHT) images previously published by van den Bergh & Pritchet (1989). These data strengthen the…

1995 The Astrophysical Journal
eHST 253
Dust in the Cores of Early-Type Galaxies
DOI: 10.1086/117667 Bibcode: 1995AJ....110.2027V

Franx, M.; van Dokkum, P. G.

The dust properties of all early-type galaxies imaged with the Planetary Camera of the Hubble Space Telescope in cycles I-III are examined. Dust is detected in 31 out of 64 galaxies, although the sample is biased against the detection of dust. From the distribution of observed axis ratios of the dust features it is inferred that 78% +/- 16% of ear…

1995 The Astronomical Journal
eHST 252
Canada-France Redshift Survey: Hubble Space Telescope Imaging of High-Redshift Field Galaxies
DOI: 10.1086/309677 Bibcode: 1995ApJ...451L...1S

Crampton, David; Lilly, S. J.; Hammer, F. +3 more

Hubble Space Telescope B and I images are presented of 32 galaxies with secure redshifts in the range 0.5 < z < 1.2 from the Canada-France Redshift Survey, a complete sample of galaxies with 17.5 <= IAB <= 22.5. These galaxies exhibit the same range of morphological types as seen locally, i.e., ellipticals, spirals, and irregulars. The…

1995 The Astrophysical Journal
eHST 248
The Central Region in M100: Observations and Modeling
DOI: 10.1086/176516 Bibcode: 1995ApJ...454..623K

Knapen, J. H.; de Jong, R. S.; Beckman, J. E. +2 more

We present new high-resolution observations of the central region in the late-type spiral galaxy M100 (NGC 4321) supplemented by three-dimensional numerical modeling of stellar and gas dynamics, including star formation (SF). Near-infrared imaging has revealed a small bulge of 4" effective diameter; a 60" radial length stellar bar of moderate stre…

1995 The Astrophysical Journal
eHST 241
Faintest Galaxy Morphologies From HST WFPC2 Imaging of the Hawaii Survey Fields
DOI: 10.1086/117631 Bibcode: 1995AJ....110.1576C

Cowie, Lennox L.; Hu, Esther M.; Songaila, Antoinette

We present very deep HST WFPC2 images in the F814W filter of two Hawaii Survey fields, SSA13 and SSA22. Using these data with previous ground- based imaging and spectroscopy, we compare the colors, star-forming properties, and morphologies of the faintest galaxies with a reference sample of bright nearby galaxies and analyze the changes in field g…

1995 The Astronomical Journal
eHST 239
Ultraviolet Radiation from Evolved Stellar Populations. II. The Ultraviolet Upturn Phenomenon in Elliptical Galaxies
DOI: 10.1086/175428 Bibcode: 1995ApJ...442..105D

O'Connell, Robert W.; Dorman, Ben; Rood, Robert T.

We discuss the far-ultraviolet upturn phenomenon (UVX) observed in elliptical galaxies and spiral galaxy bulges. Our premise is the the UV radiation from these systems emanates primarily from extreme horizontal branch (EHB) stars and their progeny. Such objects have zero-age horizontal branch envelope masses M_env_^0^<~0.05 M_sun_. Local exampl…

1995 The Astrophysical Journal
IUE 238
Three-dimensional magnetic reconnection and the magnetic topology of coronal mass ejection events
DOI: 10.1029/95GL00270 Bibcode: 1995GeoRL..22..869G

Hesse, M.; Gosling, J. T.; Birn, J.

Measurements of suprathermal electron fluxes in the solar wind indicate that field lines within coronal mass ejections, CMEs, near and beyond 1 AU are normally connected to the Sun at both ends. However, on occasion some field lines embedded deep within CMEs appear to be connected to the Sun at only one end. Here we propose an explanation for how …

1995 Geophysical Research Letters
Ulysses 238
Deuterium and the Local Interstellar Medium Properties for the Procyon and Capella Lines of Sight
DOI: 10.1086/176223 Bibcode: 1995ApJ...451..335L

Ayres, Thomas R.; Savage, Blair D.; Brown, Alexander +3 more

We present Goddard High-Resolution Spectrograph observations of the interstellar H I and D I Lyα lines and the Mg II and Fe II resonance lines formed along the lines of sight toward the nearby stars Procyon (3.5 pc, l = 214°, b = 13°) and Capella (12.5 pc, l = 163°, b = 5°). New observations of Capella were obtained at orbital phase 0.80, when the…

1995 The Astrophysical Journal
eHST 232
The Intermediate Stellar Mass Population in R136 Determined from Hubble Space Telescope Planetary Camera 2 Images
DOI: 10.1086/175950 Bibcode: 1995ApJ...448..179H

Holtzman, Jon A.; Lynds, Roger; Light, Robert M. +3 more

We have analyzed Hubble Space Telescope (HST) images of the compact, luminous star cluster R136 in the LMC that were taken with the refurbished HST and new Wide Field/Planetary Camera. These images allow us to examine the stellar population in a region of unusually intense star formation at a scale of 0.01 pc. We have detected stars to 23.5 in F55…

1995 The Astrophysical Journal
eHST 230