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The Compact UV Nucleus of M33
DOI: 10.1086/312113 Bibcode: 1999ApJ...519L.135D

Long, Knox S.; Dubus, Guillaume; Charles, Philip A.

The most luminous X-ray source in the Local Group is associated with the nucleus of M33. This source, M33 X-8, appears modulated by ~20% over a ~106 day period, making it unlikely that the combined emission from unresolved sources could explain the otherwise persistent ~1039 ergs s-1 X-ray flux. We present here high-resolutio…

1999 The Astrophysical Journal
eHST 9
The Gaseous Extent of Galaxies and the Origin of Lyα Absorption Systems. IV. Lyα Absorbers Arising in a Galaxy Group
DOI: 10.1086/307719 Bibcode: 1999ApJ...523...72O

Barcons, X.; Fernández-Soto, A.; Webb, J. K. +2 more

We present new Goddard High Resolution Spectrograph observations of Lyα absorption lines associated with a group of galaxies toward the QSO 1545+2101. We have identified eight distinct Lyα absorption features in the spectrum of QSO 1545+2101 at a mean redshift of =0.2648 with a velocity dispersion of 163 km s-1. A group of galaxies is d…

1999 The Astrophysical Journal
eHST 9
Variation of Thermal Structure with Height of a Solar Active Region Derived from SOHO CDS and YOHKOH BCS Observations
DOI: 10.1086/307820 Bibcode: 1999ApJ...524.1096S

Antiochos, Spiro K.; Watanabe, Tetsuya; Sterling, Alphonse C. +2 more

We present observations of NOAA solar Active Region 7999 when it was near the west solar limb on 1996 December 2 and 3, using data from the Coronal Diagnostic Spectrometer (CDS) experiment on the SOHO satellite. Ratios of intensities of 2 MK material (as observed in CDS Fe XVI images) to 1 MK material (from CDS Mg IX images) indicate that there is…

1999 The Astrophysical Journal
SOHO 8
Spatially Resolved Hopkins Ultraviolet Telescope Spectra of NGC 1068
DOI: 10.1086/307957 Bibcode: 1999ApJ...526..130G

Kriss, Gerard A.; Espey, Brian R.; Grimes, John P.

We present spatially resolved far-ultraviolet spectra (912-1840 Å) of NGC 1068 obtained using the Hopkins Ultraviolet Telescope (HUT) during the 1995 March Astro-2 mission. Three spectra of this prototypical Seyfert 2 galaxy were obtained through a 12" diameter aperture centered on different locations near the nucleus. The first pointing (A1) was …

1999 The Astrophysical Journal
eHST 8
First Observations of an R Coronae Borealis Star with the Space Telescope Imaging Spectrograph: RY Sagittarii near Maximum Light
DOI: 10.1086/307028 Bibcode: 1999ApJ...515..351C

Woitke, P.; Clayton, Geoffrey C.; Asplund, Martin +3 more

We describe the far-UV (1140-1740 Å) spectrum of the hydrogen-deficient R Coronae Borealis (RCB) star RY Sgr, obtained near maximum light (pulsational phase ~0.1) by the Space Telescope Imaging Spectrograph (STIS) on Hubble Space Telescope. The far-UV spectrum shows a photospheric continuum rising steeply toward longer wavelengths and two prominen…

1999 The Astrophysical Journal
eHST 8
Interacting and Interplanetary Protons Accelerated on Diverging Magnetic Field Lines: Stochastic Acceleration
DOI: 10.1086/307582 Bibcode: 1999ApJ...521..898K

Laitinen, T.; Torsti, J.; Mäkelä, P. +2 more

We study the ratio of the numbers of interplanetary to interacting protons, Γ, using a model of stochastic acceleration on open magnetic field lines in solar corona. The impact of diverging coronal magnetic field lines is incorporated into the particle transport operator and shown to be unavoidable, no matter how small the mean free path may be. W…

1999 The Astrophysical Journal
SOHO 8
Hubble Space Telescope Faint Object Spectrograph Observations of a Unique Grouping of Five QSOs: The Sizes and Shapes of Low-z Lyα Forest Absorbers
DOI: 10.1086/307692 Bibcode: 1999ApJ...522..627M

Turnshek, David A.; Monier, Eric M.; Hazard, Cyril

Observations of QSO pairs suggest that the structures responsible for Lyα forest absorption lines must have radii of hundreds of kiloparsecs if they are spherical or disklike in shape. However, only observations of groups of three or more QSOs closely spaced on the sky provide a way to measure their transverse sizes/characteristic clustering lengt…

1999 The Astrophysical Journal
eHST 8
Hubble Space Telescope NICMOS Observations of Rest-Frame Optical Continuum and Hα+[N I] Emission In FSC 10214+4724
DOI: 10.1086/307279 Bibcode: 1999ApJ...518..145E

Armus, L.; Scoville, N. Z.; Soifer, B. T. +4 more

High-resolution 1.10, 2.05, 2.12, and 2.15 µm imaging of the gravitationally lensed system FSC 10214+4724 are presented. These data extend Hubble Space Telescope (HST) observations of the lens system to redder wavelengths, thus providing the highest resolution images to date of the rest-frame optical and narrow-line (i.e., Hα+[N II]) regions…

1999 The Astrophysical Journal
eHST 8
Absorption/Emission of Solar p-Modes: Michelson Doppler Interferometer/SOHO Observations
DOI: 10.1086/307038 Bibcode: 1999ApJ...515..832H

Zweibel, Ellen G.; Jain, Rekha; Haber, Deborah

We search for sources and sinks of solar p-mode waves by creating absorption maps from Dopplergrams taken by the Michelson Doppler Interferometer instrument on board SOHO. Although the maps are noisy, we present evidence for sources and sinks, of duration ~0.5-1 hour or less, based on an autocorrelation analysis of maps made from sequential interv…

1999 The Astrophysical Journal
SOHO 8
Distances to the High Galactic Latitude Molecular Clouds G192-67 and MBM 23-24
DOI: 10.1086/307113 Bibcode: 1999ApJ...516..243G

Burrows, David N.; Grant, Catherine E.

We report on distance determinations for two high-Galactic latitude cloud complexes, G192-67 and MBM 23-24. No distance determination exists in the literature for either cloud. Thirty-four early-type stars were observed toward the two clouds, more than half of which have parallaxes measured by the Hipparcos satellite. For the remaining stars, we h…

1999 The Astrophysical Journal
Hipparcos 7