Search Publications

Ultraviolet Spectrophotometry of Variable Early-Type Be and B Stars Derived from High-Resolution IUE Data
DOI: 10.1086/323846 Bibcode: 2001ApJ...562..998S

Smith, Myron A.

High-dispersion IUE data encode significant information about aggregate line absorptions that cannot be conveniently extracted from individual stellar spectra. Here we apply a new technique in which fluxes from each echelle order of a short-wavelength IUE spectrum are binned together to construct low-resolution spectra of a rapidly varying B or Be…

2001 The Astrophysical Journal
IUE 17
First Detections of Molecular Gas Associated with the Wolf-Rayet Ring Nebula NGC 3199
DOI: 10.1086/323950 Bibcode: 2001ApJ...563..875M

Marston, A. P.

This paper presents the first observations of molecular gas associated with the Wolf-Rayet ring nebula NGC 3199 around the WR star WR 18. This includes first observations of the molecules HCN, HCO+, CN, and HNC seen in any Wolf-Rayet ring nebula. Our observations immediately suggest the presence of high-density molecular gas (>10

2001 The Astrophysical Journal
Hipparcos 17
Search for a Near-Infrared Counterpart to the Cassiopeia A X-Ray Point Source
DOI: 10.1086/322459 Bibcode: 2001ApJ...558..270K

Kulkarni, S. R.; Kaplan, D. L.; Murray, S. S.

We report deep near-infrared and optical observations of the X-ray point source in the Cassiopeia A supernova remnant, CXO J232327.9+584842. We have identified a J=21.4+/-0.3 mag and a Ks=20.5+/-0.3 mag source within the 1 σ error circle, but we believe this source is a foreground Population II star with Teff=2600-2800 K at a…

2001 The Astrophysical Journal
eHST 17
Ionization, Extinction, and Spiral Structure in the Inner Disk of NGC 1068
DOI: 10.1086/318302 Bibcode: 2001ApJ...546..866B

Smith, A. M.; Landsman, Wayne; Bruhweiler, Fred C. +2 more

We present our analysis of Hubble Space Telescope/Planetary Camera narrow-bandpass and broadband imagery of the inner 3 kpc region of NGC 1068. Our analysis of F160BW and F547M broadband continuum imagery suggests that roughly 40% of the scattered active galactic nucleus (AGN) continuum emission originates from an unobscured single cloud complex l…

2001 The Astrophysical Journal
eHST 17
The Interstellar Medium Interactions of a Runaway Luminous Blue Variable Nebula in the Large Magellanic Cloud
DOI: 10.1086/320341 Bibcode: 2001ApJ...552L.155D

Danforth, Charles W.; Chu, You-Hua

New observations of the Magellanic Cloud luminous blue variable candidate S119 (HD 269687) show the relationship of the star to its environs. Echelle spectroscopy and high-resolution Hubble Space Telescope imagery reveal an expanding bubble centered on the star. This bubble appears in both Hα and [N II] and is noticeably brighter on the near (blue…

2001 The Astrophysical Journal
eHST 17
Active Region Transient Events Observed with TRACE
DOI: 10.1086/338737 Bibcode: 2001ApJ...563L.173S

Reeves, Katharine K.; Golub, Leon; Winebarger, Amy R. +3 more

Nearly all active region observations made by the Transition Region and Coronal Explorer (TRACE) contain seemingly spontaneous, short-lived brightenings in small-scale loops. In this paper, we present an analysis of these brightenings using high-cadence TRACE observations of Active Region 9506 on 2001 June 21 from 15:17:00 to 15:46:00 UT. During t…

2001 The Astrophysical Journal
SOHO 17
Extreme Ultraviolet Explorer Observations of λ Andromedae
DOI: 10.1086/321399 Bibcode: 2001ApJ...554.1079S

Sanz-Forcada, J.; Dupree, A. K.; Brickhouse, N. S.

Extreme-ultraviolet spectra (70-740 Å) and light curves (75-175 Å) of the spectroscopic binary system λ Andromedae (HD 222107) were obtained with the Extreme Ultraviolet Explorer (EUVE) satellite in 1997 July and August. Two flares were detected during the observations that spanned 15 days, or almost 3/4 of the orbital period of 20.5 days, with a …

2001 The Astrophysical Journal
IUE 17
Hot Outflowing Gas from the X-Ray Binary Hercules X-1
DOI: 10.1086/323850 Bibcode: 2001ApJ...562..925B

Boroson, Bram; Kallman, Timothy; Vrtilek, Saeqa Dil

We present a unified picture of outflowing gas from the X-ray binary system Hercules X-1/HZ Herculis. We suggest that the outflowing gas (a wind) causes UV emission seen in mid-eclipse, narrow UV absorption lines, and broad UV P Cygni lines. Observations with the FOS and STIS spectrographs on the Hubble Space Telescope (HST) show UV emission lines…

2001 The Astrophysical Journal
eHST 16
Connecting the Sun and the Solar Wind: Comparison of the Latitudinal Profiles of Coronal and Ulysses Measurements of the Fast Wind
DOI: 10.1086/319172 Bibcode: 2001ApJ...549L.253H

Habbal, Shadia Rifai; Woo, Richard

A quantitative comparison of the latitudinal profile of polarized brightness (pB) measurements nearest the Sun at 1.15 Rsolar by the Mauna Loa Solar Observatory K-Coronameter and Ulysses interplanetary measurements of the fast solar wind during its first south polar pass, at the declining phase of the solar cycle, is made for the first …

2001 The Astrophysical Journal
Ulysses 16
Long-Slit Observations of Extended C II λ1335 Emission around V854 Centauri and RY Sagittarii
DOI: 10.1086/323065 Bibcode: 2001ApJ...560..986C

Clayton, G. C.; Ayres, T. R.

We have obtained long-slit far-ultraviolet (1150-1730 Å) spectra of the R Coronae Borealis (RCB) stars V854 Cen and RY Sgr near maximum light and pulsational phase zero with the Space Telescope Imaging Spectrograph on board the Hubble Space Telescope. The far-UV spectrum of each star shows a photospheric continuum rising steeply toward longer wave…

2001 The Astrophysical Journal
eHST 16