Search Publications

Imaging of Four Planetary Nebulae in the Magellanic Clouds Using the Hubble Space Telescope Faint Object Camera
DOI: 10.1086/186572 Bibcode: 1992ApJ...398L..41B

Boksenberg, A.; Barbieri, C.; Weigelt, G. +18 more

Using the Faint Object Camera on-board the Hubble Space Telescope, we have obtained images of four planetary nebulae (PNe) in the Magellanic Clouds, namely N2 and N5 in the SMC and N66 and N201 in the LMC. Each nebula was imaged through two narrow-band filters isolating [O III] λ5007 and Hβ, for a nominal exposure time of 1000 s in each filter. Si…

1992 The Astrophysical Journal
eHST 25
The Ionizing Radiation Field of NGC 4388 and Its Relation to the Extranuclear Emission-Line Regions
DOI: 10.1086/170992 Bibcode: 1992ApJ...386...59C

Colina, Luis

New long-slit spectroscopic observations of NGC 4388 and the extranuclear emission line regions around it are used to investigate the characteristics of the ionizing source and the structure of the extended emission-line regions. The measured luminosity of the [Fe VII) λ6087 emission line detected in the nucleus of NGC 4388 is interpreted as evide…

1992 The Astrophysical Journal
IUE 22
From Fairall 9 to High-z Objects: Pattern of Change in Ionization Structure
DOI: 10.1086/171406 Bibcode: 1992ApJ...392...74Z

Zheng, Wei; Binette, Luc; Fang, Li-Zhi

A study of 79 IUE spectra of the Seyfert galaxy Fairall 9 shows a considerable change in the continuum shape which can be characterized by several sections. The flux at 3075 A changes in approximate proportion to the optical and X-ray flux, suggesting that they may be a part of the power law. The apparent fourfold change in the continuum slope bet…

1992 The Astrophysical Journal
IUE 21
Hubble Space Telescope FOS Observations of KPD 0005+5106: A Subluminous WN-WC Descendant with Ongoing Mass Outflow?
DOI: 10.1086/186521 Bibcode: 1992ApJ...396L..79S

Sion, Edward M.; Downes, Ronald A.

The results are reported of spectroscopic observations of the ultrahigh excitation, helium-rich, prewhite-dwarf KPD 0005 + 5106 obtained with the HST Faint Object Spectrograph (FOS) in 1991 May and July with the red (FOS/RD) and blue (FOS/BL) Digicon detectors. The data reveal a rich line spectrum both in absorption and in emission with ultra-high…

1992 The Astrophysical Journal
IUE eHST 20
The Spectra of IC 418 and IC 5117 from 1.5 to 1.75 Microns
DOI: 10.1086/170933 Bibcode: 1992ApJ...385..255Z

Kwok, Sun; Zhang, C. Y.

Near-infrared spectra of planetary nebulae IC 418 and IC 5117 in the wavelength range 1.5-1.75 microns are reported. More than 10 members of the Brackett line series are detected superposed on a strong continuum. Analysis of the spectra shows that the observed flux ratios of the Brackett lines are in good agreement with the recombination line theo…

1992 The Astrophysical Journal
IUE 20
The Unusual Ultraviolet Chromospheric Spectrum of the R Coronae Borealis Star, V854 Centauri (NSV 6708), at Minimum Light
DOI: 10.1086/186253 Bibcode: 1992ApJ...384L..19C

Judge, P. G.; Stanford, S. A.; Clayton, Geoffrey C. +2 more

Results are presented of IUE observations of a decline of the recently discovered R CrB star, V854 Cen. These observations are of particular interest because they include spectra taken at 7 mag below maximum light. The 'chromospheric' emission spectra show striking differences from UV spectra of other R CrB stars in decline. Strong emission appear…

1992 The Astrophysical Journal
IUE 20
The Ultraviolet Color Gradient in the Late-Type Spiral Galaxy M33
DOI: 10.1086/186676 Bibcode: 1992ApJ...401L..83L

O'Connell, Robert W.; Bohlin, Ralph C.; Landsman, Wayne B. +3 more

The ultraviolet surface brightness and color distributions for the late-type spiral galaxy M33 are derived from images at 1520 and 2490 A that were obtained by the Ultraviolet Imaging telescope (UIT) on the Astro Spacelab mission. although the surface brightness shows a general decline with radius, the dominant spiral arms cause significant deviat…

1992 The Astrophysical Journal
IUE 19
The Luminosity of the Double-Mode Cepheid Y Carinae
DOI: 10.1086/170974 Bibcode: 1992ApJ...385..680E

Evans, Nancy R.

IUE spectra of the double-mode Cepheid Y Carinae have been used to determine the spectral type of the binary companion. From the companion spectral type (B9.O V), the absolute magnitude of the Cepheid is found to be -2.94 mag, with an estimated uncertainty of +/-0.3. This luminosity is in good agreement with that from the period-luminosity-color r…

1992 The Astrophysical Journal
IUE 19
A Spectroscopic Search for Colliding Stellar Winds in O-Type Close Binary Systems. II. Plaskett's Star (HD 47129)
DOI: 10.1086/171712 Bibcode: 1992ApJ...396..238W

Wiggs, Michael S.; Gies, Douglas R.

New evidence for colliding winds in the massive O-type binary system Plaskett's star is reported. High S/N ratio spectra of the H-alpha and He I 6678 emission lines are presented, and their orbital phase-related variations are examined in order to derive the locations and motions of the high-density gas in the system. Radial velocity cures for sev…

1992 The Astrophysical Journal
IUE 18
EXOSAT Observations of the Be/X-Ray Binary 4U 2206+54
DOI: 10.1086/172095 Bibcode: 1992ApJ...401..678S

Saraswat, Priyamvada; Apparao, Krishna M. V.

We present the X-ray observations of the Be star binary system 4U 2206 + 54 made with the EXOSAT satellite during the period 1983-1985. The observations were carried out on three occasions, each separated by roughly a year. The source was active during the 1983 and 1985 observations and several short duration flares were observed. The spectrum, du…

1992 The Astrophysical Journal
Exosat 16