Search Publications

A search for hidden white dwarfs in the ROSAT extreme ultraviolet survey
DOI: 10.1093/mnras/287.2.381 Bibcode: 1997MNRAS.287..381B

Barstow, M. A.; Burleigh, M. R.; Fleming, T. A.

The ROSAT Wide Field Camera survey has provided us with evidence for the existence of a previously unidentified sample of hot white dwarfs (WDs) in non- interacting binary systems, through the detection of extreme ultraviolet (EUV) and soft X-ray emission. These stars are hidden at optical wavelengths because of their close proximity to much more …

1997 Monthly Notices of the Royal Astronomical Society
IUE 42
A theoretical approach to globular cluster low main sequence stars.
Bibcode: 1997A&A...317...90A

Cassisi, S.; Castellani, V.; degl'Innocenti, S. +3 more

This paper present new evolutionary computations extending toward the lower main sequence previous computations given for globular cluster stars. We discuss the physical inputs with particular regard to the limit of the adopted usual treatment of the stellar atmosphere, which allows a tight correlation with actual stellar structures only for selec…

1997 Astronomy and Astrophysics
eHST 41
ULYSSES observations of intermittent heliospheric turbulence
DOI: 10.1016/S0273-1177(97)00290-1 Bibcode: 1997AdSpR..19..847H

Balogh, A.; Horbury, T. S.; Forsyth, R. J. +1 more

Structure function measurements of small scale magnetic field fluctuations in high speed streams emanating from the Sun's polar coronal holes are well described by a multifractal model of intermittent turbulence. We discuss structure functions and present measurements of intermittency through the transition regime - encompassing scales between wav…

1997 Advances in Space Research
Ulysses 41
[Fe IV] in the Orion Nebula
DOI: 10.1086/310437 Bibcode: 1997ApJ...474L.131R

Martin, P. G.; O'Dell, C. R.; Dufour, R. J. +6 more

Using the Goddard High-Resolution Spectrograph on the Hubble Space Telescope, we measured the flux of [Fe IV] (3d5 4P5/2 --> 3d5 6S5/2) λvac = 2836.56 Å in the Orion Nebula, the first detection of an [Fe IV] line in an H II region. A useful upper limit is set on the su…

1997 The Astrophysical Journal
eHST 41
Mesures de vitesses radiales. VIII. Accompagnement AU sol du programme d'observation du satellite HIPPARCOS
Bibcode: 1997A&AS..124..255F

Duflot, M.; Burnage, R.; Genty, V. +2 more

We publish 1879 radial velocities of stars distributed in 105 fields of 4^{\circ} \times 4^{\circ}. We continue the PPO series \cite[(Fehrenbach et al. 1987;]{Feh87} \cite[Duflot et al. 1990, 1992 and 1995),]{Du90} using the Fehrenbach objective prism method. Table 1 only available in electronic form at CDS via to cdsarc.u-strasbg.fr (130.79.128.5…

1997 Astronomy and Astrophysics Supplement Series
Hipparcos 41
The gravitational lensing nature of the Cloverleaf unveiled in CO (7-6) line emission.
Bibcode: 1997A&A...321...24A

Antonucci, R.; Tacconi, L.; Alloin, D. +2 more

We report 0.5" resolution imaging of the Cloverleaf quasar in the CO(7-6) line and 1.3mm continuum,, as well as 1" resolution imaging in the CO(3-2) line, performed with the IRAM interferometer. The CO(7-6) image is clearly resolved into 4 spots, demonstrating that the CO emission is also gravitationally lensed. We do not find any convincing evide…

1997 Astronomy and Astrophysics
eHST 41
Influence of heavy ions on the high-speed solar wind
DOI: 10.1029/97JA01448 Bibcode: 1997JGR...10217419L

Li, Xing; Habbal, Shadia R.; Esser, Ruth +1 more

We present the results of a parameter study of the influence of heavy ions on the background solar wind, choosing doubly ionized helium, or alpha particles, and O+6, as examples. Using a three-fluid solar wind model, we keep the input parameters to the electrons and protons unchanged and investigate the effects of changing the input ene…

1997 Journal of Geophysical Research
SOHO 41
Absolute Flux Distributions of Solar Analogs from the UV to the Near-IR
DOI: 10.1086/118332 Bibcode: 1997AJ....113.1138C

Colina, Luis; Bohlin, Ralph

The 0.225-2.695mu m absolute flux distributions of the solar analogs P041C, P177D, and P330E are presented. The ultraviolet and optical wavelength range from 0.225mu m to 0.825mu m is based on high signal-to-noise spectra obtained with the HST Faint Object Spectrograph (FOS). The spectra in the near-infrared longward of 0.825mu m are scaled versio…

1997 The Astronomical Journal
eHST 40
Diffusive Shock Acceleration in Oblique Magnetohydrodynamic Shocks: Comparison with Monte Carlo Methods and Observations
DOI: 10.1086/303646 Bibcode: 1997ApJ...476..875K

Jones, T. W.; Kang, Hyesung

We report simulations of diffusive particle acceleration in oblique magnetohydrodynamical (MHD) shocks. These calculations are based on extension to oblique shocks of a numerical model for ``thermal leakage'' injection of particles at low energy into the cosmic-ray population. That technique, incorporated into a fully dynamical diffusion-convectio…

1997 The Astrophysical Journal
Ulysses 40
Nuclear Properties of Kinematically Distinct Cores
DOI: 10.1086/304979 Bibcode: 1997ApJ...491..545C

Rich, R. Michael; Carollo, C. Marcella; Danziger, I. John +1 more

We present WFPC2 F450W, F555W, and F814W photometry for three early-type galaxies with kinematically distinct cores (KDCs), namely NGC 2434, NGC 7192, and IC 4889. For these three objects we present the B, V, and I nuclear surface brightness, isophotal, B-V and V-I profiles and derive the deprojected luminosity densities. The three KDCs have nucle…

1997 The Astrophysical Journal
eHST 40