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Measuring the Hubble Constant with the Hubble Space Telescope
DOI: 10.1086/117621 Bibcode: 1995AJ....110.1476K

Freedman, Wendy L.; Mould, Jeremy R.; Kennicutt, Robert C., Jr.

The spectacular success of the Hubble Space Telescope (HST) repair mission now makes it possible to realize one of the astrophysical goals for which the HST was designed. Despite recent progress in ground-based measurements of the distance scale, the value of the Hubble constant remains uncertain at the +/- 20%-30% level. The incompatibility of hi…

1995 The Astronomical Journal
eHST 145
Local Cloud structure from HST-GHRS
Bibcode: 1995A&A...304..461L

Ferlet, R.; Vidal-Madjar, A.; Lallement, R. +2 more

Echelle spectra at high resolution (λ/{DELTA}λ= 90,000) of the nearby stars α Aql (Altaie r), α Lyr (Vega), α Cen and δ Cas, have been obtained with the Goddard High-Resolution Spectrograph (GHRS) on board the Hubble Space Telescope (HST), during the cycles 1 and 3. In all but one spectra, interstellar Fe II and Mg II absorption lines are detected…

1995 Astronomy and Astrophysics
eHST 145
Excess Hα emission in chromospherically active binaries.
Bibcode: 1995A&A...294..165M

Montes, D.; Fernandez-Figueroa, M. J.; de Castro, E. +1 more

We study the behaviour of the excess Hα emission in a sample of 51 chromospherically active binary systems (RS CVn and BY Dra classes), of different activity levels. This sample include the 27 stars analysed by Fernandez-Figueroa et al. (1994) and the new observations of 24 systems described by Montes et al. (1994b). By using the spectral subtract…

1995 Astronomy and Astrophysics
IUE 143
RE J0317-853: the hottest known highly magnetic DA white dwarf
DOI: 10.1093/mnras/277.3.971 Bibcode: 1995MNRAS.277..971B

Jordan, S.; Barstow, M. A.; O'Donoghue, D. +3 more

We report the discovery of a new highly magnetic DA white dwarf, RE J0317-853, through its detection as an EUV source by the ROSAT Wide Field Camera. A combination of far-UV and optical spectra indicates that the star has an effective temperature ~=50000K, making it the hottest known white dwarf with a measurable magnetic field. Furthermore, the m…

1995 Monthly Notices of the Royal Astronomical Society
IUE 142
The Dense Galactic Starburst NGC 3603. I. HST/FOS Spectroscopy of Individual Stars in the Core and the source of Ionization and Kinetic Energy
DOI: 10.1086/117684 Bibcode: 1995AJ....110.2235D

Walborn, Nolan R.; Drissen, Laurent; Moffat, Anthony F. J. +1 more

We present spectrograms of 14 individual luminous stars in RD 97950, the core (r≤4"=0.12 pc) of the dense galactic starburst NGC 3603, obtained with the Faint Object Spectrograph aboard the refurbished Hubble Space Telescope. In a volume of less than a cubic light year, three luminous hydrogen-rich WNL+abs stars cohabit with six O3 stars [includin…

1995 The Astronomical Journal
eHST 142
White Dwarf Standard Stars: G191-B2B, GD 71, GD 153, HZ 43
DOI: 10.1086/117606 Bibcode: 1995AJ....110.1316B

Colina, Luis; Bohlin, Ralph C.; Finley, David S.

Three additional white dwarfs, GD 71, GD 153, and HZ 43, covering a wide range in effective temperature, have been observed with HST faint object spectrograph (FOS) to check the G191 -B2B white dwarf based absolute calibration of HST instruments. The FOS spectrophotometry of the three additional white dwarfs agree with model spectra to ∼2%. The FO…

1995 The Astronomical Journal
eHST 139
Detection of Compact Ultraviolet Nuclear Emission in LINER Galaxies
DOI: 10.1086/175250 Bibcode: 1995ApJ...440...91M

Filippenko, Alexei V.; Ho, Luis C.; Maoz, Dan +4 more

Low-ionization nuclear emission-line regions (LINERs), which exist in a large fraction of galaxies, may be the least luminous manifestation of quasar activity. As such, they may make possible the study of the AGN phenomenon in the nearest galaxies. The nature of LINERs has, however, remained controversial because an AGN-like nonstellar continuum s…

1995 The Astrophysical Journal
eHST 138
Radio to X-ray energy distribution of BL Lacertae objects.
Bibcode: 1995A&AS..109..267G

Giommi, P.; Micol, A.; Ansari, S. G.

We present multifrequency spectra of a large number of radio and X-ray selected BL Lacertae objects constructed using non-simultaneous archival data. The data were obtained using the European Space Information System (ESIS) and are from several radio and optical catalogues, the IRAS Faint Source Catalogue, the Einstein and the EXOSAT databases. Th…

1995 Astronomy and Astrophysics Supplement Series
Exosat 137
Ulysses observations of Alfvén waves in the southern and northern solar hemispheres
DOI: 10.1029/95GL03268 Bibcode: 1995GeoRL..22.3381S

Balogh, A.; Smith, E. J.; Neugebauer, M. +1 more

Alfvén waves with periods from <1 to >10 hours are shown to be continuously present in the sun's south and north polar regions. Below ≈ 30° latitude, as revealed by the rapid traversal of the equatorial region by Ulysses, the wave power averaged over a solar rotation decreases abruptly. The correlations between magnetic field and solar wind …

1995 Geophysical Research Letters
Ulysses 136
HST/FOS Spectroscopy of ETA Carinae: The Star Itself, and Ejecta Within 0.3 Arcsec
DOI: 10.1086/117408 Bibcode: 1995AJ....109.1784D

Walborn, Nolan R.; Weigelt, Gerd; Humphreys, Roberta M. +4 more

Ground-based spectroscopy of η Car includes at least four components ABCD within a core region less than 0.4 across, and usually other material as well. Using the Hubble Space Telescope (HSTs) Faint Object Spectrograph (FOS), we have obtained separate data on component A and on B+C+D. Object A is found to be the central star; this is the fist time…

1995 The Astronomical Journal
eHST 135