Search Publications

The Southern High-Speed Stream: Results from the SWICS Instrument on Ulysses
DOI: 10.1126/science.7754380 Bibcode: 1995Sci...268.1033G

Livi, S.; Balsiger, H.; Geiss, J. +8 more

The high-speed solar wind streaming from the southern coronal hole was remarkably uniform and steady and was confined by a sharp boundary that extended to the corona and chromosphere. Charge state measurements indicate that the electron temperature in this coronal hole reached a maximum of about 1.5 million kelvin within 3 solar radii of the sun. …

1995 Science
Ulysses 228
The D/H and ^18^O/^16^O ratios in water from comet P/Halley.
Bibcode: 1995A&A...302..301E

Eberhardt, P.; Krankowsky, D.; Hodges, R. R. +1 more

From a detailed evaluation of the ion currents measured by the Neutral Mass Spectrometer (NMS) on the Giotto spaceprobe in the 17.5amu/e to 21.5amu/e mass range inside the contact surface of P/Halley we derive the cometary ion densities for masses 18amu/e to 21amu/e. From these we calculate the deuterium and ^18^O abundances in the H_3_O^+^ ion to…

1995 Astronomy and Astrophysics
Giotto 226
The morphological identification of the rapidly evolving population of faint galaxies
DOI: 10.1093/mnras/275.1.L19 Bibcode: 1995MNRAS.275L..19G

Ellis, Richard; Glazebrook, Karl; Griffiths, Richard +1 more

The excess numbers of blue galaxies at faint magnitudes are a long-standing cosmological puzzle. We present new number-magnitude counts as a function of galactic morphology from the first deep fields of the Cycle 4 Hubble Space Telescope Medium Deep Survey project. From a sample of 301 galaxies we define counts for elliptical, spiral and irregular…

1995 Monthly Notices of the Royal Astronomical Society
eHST 225
Spectral Classification of Galaxies: an Orthogonal Approach
DOI: 10.1086/117587 Bibcode: 1995AJ....110.1071C

Calzetti, D.; Kinney, A. L.; Connolly, A. J. +2 more

Classification of galaxy spectral energy distributions in terms of orthogonal basis functions provides an objective means of estimating the number of significant spectral components that comprise a particular galaxy type. We apply the Karhunen-Loeve transform to derive a spectral eigensystem from a sample of ten galaxy spectral energy distribution…

1995 The Astronomical Journal
IUE 220
Radiative Levitation in Hot White Dwarfs: Equilibrium Theory
DOI: 10.1086/192184 Bibcode: 1995ApJS...99..189C

Chayer, P.; Fontaine, G.; Wesemael, F.

We present the results of detailed calculations of radiative levitation in hot white dwarfs using the extensive and homogeneous atomic data given in TOPBASE. Radiative accelerations and equilibrium abundances have been computed for C, N, O, Ne, Na, Mg, Al, Si, S, Ar, Ca, and Fe on grids of pure hydrogen and pure helium stellar envelope models. The…

1995 The Astrophysical Journal Supplement Series
IUE 219
The Evolution of C/O in Dwarf Galaxies from Hubble Space Telescope FOS Observations
DOI: 10.1086/175503 Bibcode: 1995ApJ...443...64G

Terlevich, E.; Terlevich, R.; Garnett, D. R. +5 more

We present UV observations of seven H II regions in low-luminosity dwarf irregular galaxies and the Magellanic Clouds obtained with the Faint Object Spectrograph on the Hubble Space Telescope (HST) in order to measure the C/O abundance ratio in the interstellar medium (ISM) of those galaxies. We measure both O III] 1666 A and C III] 1909 A in our …

1995 The Astrophysical Journal
eHST 209
A new model for the infrared emission of quasars
DOI: 10.1093/mnras/272.4.737 Bibcode: 1995MNRAS.272..737R

Rowan-Robinson, Michael

The optical-UV continua of 75 PG quasars are modelled to test two extreme hypotheses: (a) the range of continuum shapes observed is the result of different amounts of reddening of a single underlying continuum, and (b) the range of continuum slopes is entirely intrinsic, due to accretion discs being viewed at different inclinations. Although (a) i…

1995 Monthly Notices of the Royal Astronomical Society
IUE 208
Energetic Particle Experiment ERNE
DOI: 10.1007/BF00733438 Bibcode: 1995SoPh..162..505T

Valtonen, E.; Peltonen, P.; Eronen, T. +12 more

The Energetic and Relativistic Nuclei and Electron (ERNE) experiment will investigate the solar atmosphere and the heliosphere by detecting particles produced in various kinds of energy release processes. ERNE is at the upper end in energy among the SOHO particle instruments. The instrument will measure the energy spectra of elements in the range …

1995 Solar Physics
SOHO 205
HST Imaging of Atmospheric Phenomena Created by the Impact of Comet Shoemaker-Levy 9
DOI: 10.1126/science.7871425 Bibcode: 1995Sci...267.1288H

Simon, A. A.; Beebe, R. F.; West, R. A. +14 more

Hubble Space Telescope (HST) images reveal major atmospheric changes created by the collision of comet Shoemaker-Levy 9 with Jupiter. Plumes rose to 3000 kilometers with ejection velocities on the order of 10 kilometers second-1; some plumes were visible in the shadow of Jupiter before rising into sunlight. During some impacts, the inco…

1995 Science
eHST 203
COSTEP - Comprehensive Suprathermal and Energetic Particle Analyser
DOI: 10.1007/BF00733437 Bibcode: 1995SoPh..162..483M

Sierks, H.; Kunow, H.; Müller-Mellin, R. +16 more

The COSTEP experiment on SOHO forms part of the CEPAC complex of instruments that will perform studies of the suprathermal and energetic particle populations of solar, interplanetary, and galactic origin. Specifically, the LION and EPHIN instruments are designed to use particle emissions from the Sun for several species (electrons, protons, and he…

1995 Solar Physics
SOHO 192