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Ultraviolet and Optical Observations of OB Associations in M31
DOI: 10.1086/192171 Bibcode: 1995ApJS...98..595H

O'Connell, R. W.; Bohlin, R. C.; Stecher, T. P. +7 more

Images of the central and southern parts of the local group Sb spiral galaxy M31 were obtained by the Ultraviolet Imaging Telescope during the Astro-1 Spacelab mission. Stellar photometry is obtained for 611 stars in 59 van den Bergh associations in the near-UV A1 band (central wavelength 2490 A), and for 130 of these stars in the far-UV B1 band (…

1995 The Astrophysical Journal Supplement Series
IUE 14
Properties of the +70 Kilometers per Second Cloud toward HD 203664
DOI: 10.1086/175695 Bibcode: 1995ApJ...445..314S

Sembach, Kenneth R.

I present high-resolution International Ultraviolet Explorer (IUE) spectra of the ultraviolet absorption in an intermediate-velocity interstellar cloud (nuLSR approximately equal to +70 km/s) toward HD 203664. The combined, multiple IUE images result in spectra with S/N = 15-40 and resolutions of approximately 20-25 km/s. The intermedia…

1995 The Astrophysical Journal
IUE 14
Anomalous cosmic ray oxygen and neon (∼2.4 MeV/nucl) at high southern heliolatitudes
DOI: 10.1029/95GL03551 Bibcode: 1995GeoRL..22.3353L

Lanzerotti, L. J.; Maclennan, C. G.

We report measurements of the anomalous oxygen and neon as measured with the HI-SCALE instrument on Ulysses at high southern heliolatitudes. Using both energy spectral features and C/O ratios, 2.0-2.8 MeV/nucl anomalous O is not distinguishable below a latitude of ∼40°S. The heliolatitude gradient is found to be +0.06±0.50% / degree for the heliol…

1995 Geophysical Research Letters
Ulysses 14
X-ray observations of NGC 1851 and the globular cluster LMXBs
DOI: 10.1093/mnras/273.1.201 Bibcode: 1995MNRAS.273..201C

Charles, P. A.; Callanan, P. J.; Penny, A. J.

We present new Ginga observations of the globular cluster X-ray source 4U 0513-40 in NGC 1851. Despite the 2-d time-base of the observations, no eclipsing or dipping modulation was found. The spectrum can be well modelled by a power law of index 2.1 to energies of at least 10 keV. We find from archive EXOSAT data that an additional blackbody contr…

1995 Monthly Notices of the Royal Astronomical Society
Exosat 13
Medium-Resolution Far-Ultraviolet Spectroscopy of PKS 2155-304
DOI: 10.1086/187738 Bibcode: 1995ApJ...439L..33A

Grewing, M.; Hurwitz, M.; Bowyer, S. +5 more

Using the Berkeley spectrometer of the Orbiting Retrievable Far and Extreme Ultraviolet Spectrometer (ORFEUS) we observed the 87-117 nm UV spectrum of the BL Lac object PKS 2155 - 304 with about 0.5 A resolution. In addition to the expected interstellar lines we detected higher quantum number counterparts of the intergalactic Lyα lines discovered …

1995 The Astrophysical Journal
IUE 13
The High Latitude Heliospheric Magnetic Field
DOI: 10.1007/BF00768772 Bibcode: 1995SSRv...72..153F

Forsyth, R. J.

As the Ulysses spacecraft approaches its first pass under the south pole of the sun, it is an appropriate time to review our current knowledge and predictions regarding the three dimensional behaviour of the heliospheric magnetic field, in particular at high heliographic latitudes. Optical techniques for measuring the photospheric magnetic field a…

1995 Space Science Reviews
Ulysses 13
Astrometry of 19 globular clusters.
Bibcode: 1995A&AS..112...89P

Johnston, H. M.; Picard, A.

We present accurate positions for the center of 19 globular clusters, 8 of which are known to contain X-ray sources and/or pulsars. The positions are based on a new centroiding algorithm applied to CCD images of the clusters. The fundamental astrometry is performed with plates from the ESO Schmidt telescope, using the Hipparcos Input Catalogue as …

1995 Astronomy and Astrophysics Supplement Series
Hipparcos 13
Non-standard Extinction by Circumnuclear Dust in Active Galactic Nuclei
Bibcode: 1995AcA....45..623C

Szczerba, R.; Madejski, G.; Czerny, B. +2 more

Observational data imply that Active Galactic Nuclei are likely to have a substantial amount of dust within some 0.1-100pc. This dust modifies the observed spectrum of the nucleus by reprocessing a significant fraction of its intrinsic bolometric luminosity. The details of the emerging spectrum in the infrared and in the ultraviolet are dependent …

1995 Acta Astronomica
IUE 13
Dust particles beyond the asteroid belt - a study based on recent results of the Ulysses dust experiment
DOI: 10.1016/0032-0633(95)00073-E Bibcode: 1995P&SS...43..827M

Mann, Ingrid; Grün, Eberhard

Dust fluxes detected by the Ulysses dust experiment beyond the asteroid belt, their possible sources and the possibilities of comparing them to observations of dust in the Zodiacal light are discussed. The dust fluxes detected at solar distances about r < 2.5 AU are compatible with a population of interplanetary dust particles moving on low ecc…

1995 Planetary and Space Science
Ulysses 13
Properties of the HIPPARCOS Input Catalogue
Bibcode: 1995A&A...304...82T

Evans, D. W.; Arenou, F.; Lindegren, L. +17 more

The positions, proper motions, magnitudes and colour indices contained in the Hipparcos Input Catalogue are compared with preliminary Hipparcos mission results. The Hipparcos data considered, the `combined 30-month solution', or H30, is a preliminary catalogue derived from the analysis of the first 30 months of data (out of a total of 37 months), …

1995 Astronomy and Astrophysics
Hipparcos 13