Search Publications

EIT: Extreme-Ultraviolet Imaging Telescope for the SOHO Mission
DOI: 10.1007/BF00733432 Bibcode: 1995SoPh..162..291D

Michels, D. J.; Gurman, J. B.; Delaboudinière, J. -P. +25 more

The Extreme-ultraviolet Imaging Telescope (EIT) will provide wide-field images of the corona and transition region on the solar disc and up to 1.5 R⊙ above the solar limb. Its normal incidence multilayer-coated optics will select spectral emission lines from Fe IX (171 å), Fe XII (195 å), Fe XV (284 å), and He II (304 å) to provide sensitive tempe…

1995 Solar Physics
SOHO 1687
The SOHO Mission: an Overview
DOI: 10.1007/BF00733425 Bibcode: 1995SoPh..162....1D

Domingo, V.; Fleck, B.; Poland, A. I.

The Solar and Heliospheric Observatory (SOHO) is a space mission that forms part of the Solar-Terrestrial Science Program (STSP), developed in a collaborative effort by the European Space Agency (ESA) and the National Aeronautics and Space Administration (NASA). The STSP constitutes the first "cornerstone" of ESA's long-term programme known as "Sp…

1995 Solar Physics
SOHO 1364
SUMER - Solar Ultraviolet Measurements of Emitted Radiation
DOI: 10.1007/BF00733430 Bibcode: 1995SoPh..162..189W

Vial, J. -C.; Grewing, M.; Wilhelm, K. +13 more

The instrument SUMER - Solar Ultraviolet Measurements of Emitted Radiation is designed to investigate structures and associated dynamical processes occurring in the solar atmosphere, from the chromosphere through the transition region to the inner corona, over a temperature range from 104 to 2 × 106K and above. These observat…

1995 Solar Physics
SOHO 837
The Coronal Diagnostic Spectrometer for the Solar and Heliospheric Observatory
DOI: 10.1007/BF00733431 Bibcode: 1995SoPh..162..233H

Mason, H. E.; Harrison, R. A.; Fludra, A. +36 more

The Coronal Diagnostic Spectrometer is designed to probe the solar atmosphere through the detection of spectral emission lines in the extreme ultraviolet wavelength range 150 - 800 å. By observing the intensities of selected lines and line profiles, we may derive temperature, density, flow and abundance information for the plasmas in the solar atm…

1995 Solar Physics
SOHO 648
The Centers of Early-Type Galaxies with HST.I.An Observational Survey
DOI: 10.1086/117719 Bibcode: 1995AJ....110.2622L

Faber, S. M.; Dressler, A.; Byun, Y. -I. +6 more

We have obtained V-band images of 45 nearby elliptical galaxies and bulges using the original Planetary Camera of the Hubble Space Telescope. The majority of the sample is at distances of 10-20 Mpc. This represents a substantial increase in the number of galaxies that have been studied at a resolution of a few parsecs. At this resolution, many gal…

1995 The Astronomical Journal
eHST 621
Hubble Space Telescope Observations of Young Star Clusters in NGC 4038/4039, "The Antennae" Galaxies
DOI: 10.1086/117334 Bibcode: 1995AJ....109..960W

Whitmore, Bradley C.; Schweizer, Francois

New, high-resolution images of the disks of NGC 4038/4039 obtained with the Wide Field Camera of the Hubble Space Telescope (HST) are presented. NGC 4038/4039, nicknamed "The Antennae," is a prototypical example of a pair of colliding galaxies believed to be at an early stage of a merger. Down to the limiting magnitude of V~23 mag, the HST images …

1995 The Astronomical Journal
eHST 582
Starbursts and Star Clusters in the Ultraviolet
DOI: 10.1086/117721 Bibcode: 1995AJ....110.2665M

Leitherer, C.; Garnett, D. R.; Heckman, T. M. +3 more

We present ultraviolet (UV) images of nine starburst galaxies obtained with the Hubble Space Telescope using the Faint Object Camera. The galaxies range in morphology from blue compact dwarfs to ultraluminous merging far-infrared galaxies. Our data combined with new and archival UV spectroscopy and far-infrared fluxes allow us to dissect the anato…

1995 The Astronomical Journal
IUE eHST 556
The Ultraviolet Coronagraph Spectrometer for the Solar and Heliospheric Observatory
DOI: 10.1007/BF00733433 Bibcode: 1995SoPh..162..313K

Livi, S.; Romoli, M.; Geiss, J. +37 more

The SOHO Ultraviolet Coronagraph Spectrometer (UVCS/SOHO) is composed of three reflecting telescopes with external and internal occultation and a spectrometer assembly consisting of two toric grating spectrometers and a visible light polarimeter. The purpose of the UVCS instrument is to provide a body of data that can be used to address a broad ra…

1995 Solar Physics
SOHO 457
The IUE Survey for Damped Lyman- alpha and Lyman-Limit Absorption Systems: Evolution of the Gaseous Content of the Universe
DOI: 10.1086/175286 Bibcode: 1995ApJ...440..435L

Turnshek, David A.; Lanzetta, Kenneth M.; Wolfe, Arthur M.

We present a spectroscopic survey for moderate-redshift absorption features from damped Lyα and Lyman- limit absorption systems. The survey is based on a set of optimally extracted and co-added International Ultraviolet Explorer spectra of QSOs, BL Lac objects, and Seyfert galaxies. Results of this survey are combined with those of previous survey…

1995 The Astrophysical Journal
IUE 359
Software for the Analysis of Emission Line Nebulae
DOI: 10.1086/133637 Bibcode: 1995PASP..107..896S

Shaw, Richard A.; Dufour, Reginald J.

A set of software tools has been developed for the IRAF/STSDAS environment to derive the physical conditions in a low-density (nebular) gas given appropriate diagnostic emission line ratios; and lien emissivities given appropriate emission line fluxes, the electron temperature (T_e) and density (N_e). The package is based on the five-level program…

1995 Publications of the Astronomical Society of the Pacific
IUE 341