Search Publications

Search for Interstellar Water in the Translucent Molecular Cloud toward HD 154368
DOI: 10.1086/306033 Bibcode: 1998ApJ...503..780S

Stauffer, John; Neufeld, David; Melnick, Gary J. +2 more

We report an upper limit of 9 × 1012 cm-2 on the column density of water in the translucent cloud along the line of sight toward HD 154368. This result is based on a search for the C-X band of water near 1240 Å carried out using the Goddard High-Resolution Spectrograph (GHRS) of the Hubble Space Telescope. Our observational l…

1998 The Astrophysical Journal
eHST 13
WFPC2 Observations of NGC 454: An Interacting Pair of Galaxies
DOI: 10.1086/311115 Bibcode: 1998ApJ...492L.135S

Panagia, N.; Stiavelli, M.; Romaniello, M. +3 more

We present Wide Field Planetary Camera 2 images in the F450W, F606W, and F814W filters of the interacting pair of galaxies NGC 454. Our data indicate that the system is in the early stages of interaction. A population of young star clusters has formed around the late component, and substantial amounts of gas have sunk into the center of the earlie…

1998 The Astrophysical Journal
eHST 13
A Fit to the Simultaneous Broadband Spectrum of Cygnus X-1 Using the Transition Disk Model
DOI: 10.1086/305278 Bibcode: 1998ApJ...495..407M

Misra, R.; Melia, Fulvio; Chitnis, V. R.

We have used the transition disk model to fit the simultaneous broadband (2-500 keV) spectrum of Cygnus X-1 from OSSE and Ginga observations. In this model, the spectrum is produced by saturated Comptonization within the inner region of the accretion disk, where the temperature varies rapidly with radius. In an earlier attempt, we demonstrated the…

1998 The Astrophysical Journal
Exosat 13
Kinematics of the narrow-line region of NGC 1068
Bibcode: 1998A&A...338..405D

Dietrich, M.; Wagner, S. J.

We investigated the kinematics of the Narrow Line Region of NGC 1068. In order to study the kinematics and to determine whether the unusual broad line width can be attributed to motion of NLR clouds in a deep gravitational potential or to expanding shocks, we carried out spatially resolved echelle spectroscopy. High spectral resolution enables the…

1998 Astronomy and Astrophysics
eHST 13
Dust in LBV Nebulae
DOI: 10.1023/A:1001145110961 Bibcode: 1998Ap&SS.255..179W

Waters, L. B. F. M.; Morris, P. W.; Lamers, H. J. G. L. M. +2 more

1998 Astrophysics and Space Science
ISO 13
Hubble Space Telescope Astrometric Observations and Orbital Mean Motion Corrections for the Inner Uranian Satellites
DOI: 10.1086/300245 Bibcode: 1998AJ....115.1190P

Pascu, Dan; Rohde, James R.; Seidelmann, P. Kenneth +6 more

The 10 small inner satellites of Uranus were discovered in 1986 with Voyager 2 and not seen again until 1994, when eight were recovered with the Hubble Space Telescope Wide Field Planetary Camera 2 for astrometric, dynamical, and photometric studies. Thirty-three exposures were taken on 1994 August 14 with the PC1 chip in the BVRI filters. Measura…

1998 The Astronomical Journal
eHST 13
Limits on the Boron Isotopic Ratio in HD 76932
DOI: 10.1086/306315 Bibcode: 1998ApJ...507..387R

Rebull, Luisa; Duncan, Douglas; Johansson, Sveneric +2 more

Data in the λ2090 B region of HD 76932 have been obtained at a high signal-to-noise ratio using the Hubble Space Telescope Goddard High-Resolution Spectrograph echelle at a resolution of 90,000. This wavelength region has been previously identified as a likely candidate for observing the 11B/10B isotopic splitting. The observ…

1998 The Astrophysical Journal
eHST 13
NGC 5252 - a Liner undercover
DOI: 10.48550/arXiv.astro-ph/9802068 Bibcode: 1998A&A...333..877G

Goncalves, A. C.; Veron, P.; Veron-Cetty, M. -P.

Ground based long slit spectroscopic observations of the nuclear region of NGC 5252, and Hubble Space Telescope (HST) Faint Object Spectrograph (FOS) spectra of the nucleus and two bright knots located 0.36'' NE and 0.31'' SW from it, show that the nuclear region exhibits the characteristics of a Liner with exceptionally strong [O i] emission, all…

1998 Astronomy and Astrophysics
eHST 13
Far-Ultraviolet and Visible Imaging of the Nucleus of M32
DOI: 10.1086/306169 Bibcode: 1998ApJ...505..230C

Casertano, Stefano; Cole, Andrew A.; Ballester, Gilda E. +15 more

We have imaged the nucleus of M32 at 1600 Å (FUV) and 5500 Å (V) using the Wide-Field/Planetary Camera 2 (WFPC2) aboard the Hubble Space Telescope. We detected the nucleus at 1600 Å using the redleak-free Woods filter on WFPC2. The far-ultraviolet (FUV) light profile can be fitted with a Gaussian of FWHM 0.46" (4.6 pixels) but cannot be resolved i…

1998 The Astrophysical Journal
eHST 13
Infrared Observations of the Transition from Chaotic to Crystalline Silicates via Thermal Annealing in the Laboratory
DOI: 10.1023/A:1001597406360 Bibcode: 1998Ap&SS.255..427H

Hallenbeck, S.; Nuth, J.

1998 Astrophysics and Space Science
ISO 13