Search Publications

Disk-Overflow Accretion in GK Persei?
DOI: 10.1086/187274 Bibcode: 1994ApJ...424L..57H

Hellier, Coel; Livio, Mario

We reanalyze the 1983 European X-ray Observatory Satellite (EXOSAT) observations of GK Per during an outburst to investigate the approximately 5000 s quasiperiodic modulation. We find that the spectral behavior is reminiscent of dipping low-mass X-ray binaries and note that the time scale is characteristic of the radius where an accretion stream o…

1994 The Astrophysical Journal
Exosat 21
Ultraviolet Light Curves of beta Lyrae: Comparison of OAO A-2, IUE, and Voyager Observations
DOI: 10.1086/173691 Bibcode: 1994ApJ...421..787K

Kondo, Yoji; Polidan, Ronald S.; Eaton, Joel A. +3 more

The six-band ultraviolet light curves of beta Lyrae obtained with the Orbiting Astronomical Observatory (OAO) A-2 in 1970 exhibited a very unusual behavior. The secondary minimum deepened at shorter wavelength, indicating that one was not observing light variations caused primarily by the eclipses of two stars having a roughly Planckian energy dis…

1994 The Astrophysical Journal
IUE 21
Emission Lines in the Long-Period Cepheid L Carinae
DOI: 10.1086/173570 Bibcode: 1994ApJ...420..401B

Bohm-Vitense, Erika; Love, Stanley G.

For the Cepheid l Carinae, with a pulsation period of 35.5 days, we have studied the emission-line fluxes as a function of pulsational phase in order to find out whether we see chromospheric and transition-layer emission due to an outward-moving shock. All emission lines show a steep increase in flux shortly before maximum light, suggestive of a s…

1994 The Astrophysical Journal
IUE 21
The Hubble Space Telescope Extragalactic Distance Scale Key Project. II. Photometry of WFC Images of M81
DOI: 10.1086/174227 Bibcode: 1994ApJ...428..143H

Illingworth, Garth D.; Madore, Barry F.; Freedman, Wendy L. +11 more

The Extragalactic Distance Scale (H_0_) Key Project for Hubble Space Telescope (HST) aims to employ the Cepheid period-luminosity (P-L) relation to measure galaxy distances out as far as the Virgo Cluster. The vital steps in this program are (1) to obtain precise photometry of stellar images from the Wide Field Camera (WFC) exposures of selected g…

1994 The Astrophysical Journal
eHST 21
IUE Spectra and Optical Imaging of the Oxygen-rich Supernova Remnant N132D
DOI: 10.1086/173811 Bibcode: 1994ApJ...423..334B

Blair, William P.; Raymond, John C.; Long, Knox S.

We present new optical Charge Coupled Devices (CCD) interference filter imagery and International Ultraviolet Explorer (IUE) spectroscopy for the oxygen-rich supernova remnant N132D in the Large Magellanic Cloud. The optical images show a wealth of structure, and comparison with an archival Einstein High Resolution Imager (HRI) X-ray image shows t…

1994 The Astrophysical Journal
IUE 21
The Optical--Ultraviolet--Gamma-Ray Spectrum of 3C 279
DOI: 10.1086/174393 Bibcode: 1994ApJ...430..191N

Kazanas, D.; Ferland, G. J.; Browne, I. W. A. +6 more

We have obtained spectroscopy of the violently variable quasar 3C 279, simultaneous with γ-ray observations, in 1992 April. Our combined optical (McDonald Observatory and CTIO) and ultraviolet (HST) observations, made when the source was faint, show a very steep power-law continuum (Fnu_ is proportional to ν^-1.95^), and strong broad em…

1994 The Astrophysical Journal
eHST 21
The Nuclear Colors and Morphology of Field Galaxies at Moderate Redshift
DOI: 10.1086/187672 Bibcode: 1994ApJ...437L..17F

Illingworth, Garth D.; Forbes, Duncan A.; Koo, David C. +2 more

Until recently, the study of faint field galaxies has been limited by the spatial resolutions available to ground-based imaging. Here we present HST images with 0-1 resolution for a sample of 203 field galaxies with I <= 22 (corresponding to B <= 24.5). The expected median redshift for such a sample is z ~ 0.5. The high resolution of HST all…

1994 The Astrophysical Journal
eHST 20
The He i lambda 10830 Line in Classical Cepheids. I. Observations
DOI: 10.1086/173856 Bibcode: 1994ApJ...423..777S

Sasselov, Dimitar D.; Lester, John B.

Using the Fourier Transform Spectrometer at the Canada-France-Hawaii telescope, we obtained high- resolution, high signal-to-noise ratio spectra of seven classical Cepheids at 1.08 µm. We report the first certain detection of the He I λ10830 line in Cepheids. Three of the Cepheids, X Sgr, η Aql, and ζ Gem, were observed with full phase cover…

1994 The Astrophysical Journal
IUE 20
The Pursuit of Heavy Elements in the HgMn-Type Star chi Lupi: Observations with the GHRS in the COSTAR ERA
DOI: 10.1086/187596 Bibcode: 1994ApJ...435L..67W

Gilliland, Ronald L.; Lindler, Don J.; Wahlgren, Glenn M. +4 more

Observations of the ultra-sharp-lined HgMn star Chi Lupi made with the Goddard High Resolution Spectrograph (GHRS) after the Hubble Space Telescope (HST) First Servicing Mission display the effect of the Corrective Optics Space Telescope Axial Replacement instrument (COSTAR) upon the spectral resolution of several observing modes. The resolution i…

1994 The Astrophysical Journal
eHST 20
HST Observations of the [O iii] Emission-Line Region in Markarian 78
DOI: 10.1086/173627 Bibcode: 1994ApJ...421...87C

Boksenberg, A.; Capetti, A.; Sparks, W. B. +1 more

We present the results of HST observations of Mrk 78, a Seyfert 2 galaxy. Observations were taken with the Faint Object Camera using the F550M, F502M (which includes the [O III] λλ4959, 5007 emission lines), and F130M filters. These are medium band filters centered at 5500, 5020, and 1300 A, respectively. The [O III] image shows a biconical shape …

1994 The Astrophysical Journal
eHST 19