Search Publications

First Results from the Space Telescope Imaging Spectrograph: Optical Spectra of Gliese 229B
DOI: 10.1086/311103 Bibcode: 1998ApJ...492L.181S

Moos, H. W.; Bruhweiler, F. C.; Maran, S. P. +12 more

We report the first Hubble Space Telescope Space Telescope Imaging Spectrograph (STIS) CCD spectroscopy of the bona fide brown dwarf Gliese 229B. The optical spectrum shows absorptions of Cs I at 8944 Å and water vapor bands at 9300-9600 Å. Strong CaH, FeH, TiO, and VO bands observed in late M dwarfs are absent from the spectrum of Gliese 229B. Th…

1998 The Astrophysical Journal
eHST 35
Lyα Absorption Systems and the Nearby Galaxy Distribution
DOI: 10.1086/306208 Bibcode: 1998ApJ...505..506G

Grogin, Norman A.; Geller, Margaret J.

We study the galaxy number density (smoothed on a 5 h-1 Mpc scale) around 18 low-redshift Lyα absorbers previously observed with HST. The absorbers lie in the foregrounds of Mrk 335, Mrk 421, Mrk 501, I Zw 1, and 3C 273, all within regions where there are now complete redshift surveys to mZw = 15.5. We construct a smoothed ga…

1998 The Astrophysical Journal
eHST 35
Hubble Space Telescope Observations of the Gravitationally Lensed Cloverleaf Broad Absorption Line QSO H1413+1143: Spectroscopy of the Lyα Forest and Metal-Line Systems
DOI: 10.1086/305372 Bibcode: 1998ApJ...496..177M

Turnshek, David A.; Monier, Eric M.; Lupie, Olivia L.

The intervening Lyα forest and metal-line absorbers toward the ``Cloverleaf'' gravitational lens H1413+1143 (zem = 2.54, mv ~ 17) are examined along the four individual sight lines using HST-FOS spectra. The observations probe the Lyα forest systems on size scales of up to 4 h-1 kpc (H0 = 100 h km s

1998 The Astrophysical Journal
eHST 35
Abundances of UV bright stars in globular clusters. I. ROA 5701 in omega Centauri and Barnard 29 in M 13
DOI: 10.48550/arXiv.astro-ph/9809128 Bibcode: 1998A&A...339..537M

Heber, U.; Moehler, S.; Lemke, M. +1 more

Two UV brights stars in globular clusters, ROA 5701 (omega Cen) and Barnard 29 (M 13) are analysed from high-resolution UV and optical spectra. The main aim is the measurement of iron abundances from UV spectra obtained with the HST-GHRS. In addition atmospheric parameters and abundances for He, C, N, O, and Si are derived from optical spectra (ES…

1998 Astronomy and Astrophysics
IUE eHST 35
New Hubble Space Telescope Observations of High-Velocity Lyα and Hα in SNR 1987A
DOI: 10.1086/311780 Bibcode: 1998ApJ...509L.117M

Filippenko, Alexei V.; Pun, C. S. J.; Garnavich, Peter +12 more

We describe and model high-velocity (~15,000 km s-1) Lyα and Hα emission from the supernova remnant SNR 1987A seen in 1997 September and October with the Space Telescope Imaging Spectrograph. Part of this emission comes from a reverse shock located at ~75% of the radius of the inner boundary of the inner circumstellar ring and confined …

1998 The Astrophysical Journal
eHST 35
The spectral variability of the cool hypergiant rho Cassiopeiae
Bibcode: 1998A&A...330..659L

Lobel, A.; Parker, J. Wm.; de Jager, C. +3 more

We checked the change of the effective temperature with the atmospherical pulsation of rho Cas from combined analyses of optical spectra of 1993-95 and IUE spectra of 1979-81. We find an upper range for bigtriangleup T_eff =~ 750 K over a period of 16-17 months. We present a thorough study of the related absorption line profile changes from which …

1998 Astronomy and Astrophysics
IUE 35
HS0507+0434: a double DA degenerate with a ZZCeti component
Bibcode: 1998A&A...330..277J

Reimers, D.; Dreizler, S.; Heber, U. +6 more

HS0507+0434 and HS2240+1234 are two new common proper motion pairs of DA white dwarfs, discovered by the Hamburg Quasar Survey. Our model atmosphere analysis shows that HS0507+0434A has an effective temperature of 20000K and is remarkably young (tau_cool < 1Gyr) compared to the average cooling time of all known wide double degenerates (~ 3Gyr).…

1998 Astronomy and Astrophysics
IUE 35
Infrared lasers in the circumstellar disk of MWC 349
Bibcode: 1998A&A...333L..63T

Quirrenbach, A.; Martin-Pintado, J.; Thum, C. +1 more

Observations of hydrogen recombination lines were made with the Infrared Space Observatory (ISO) towards the star MWC349, where the alpha -transitions at short millimeter and submillimeter wavelengths have been found to be masers. All alpha -line s in the ISO wavelength range from 2.4 to 190mu m (quantum numbers n=4 to 15) were detected. We find t…

1998 Astronomy and Astrophysics
ISO 35
A new determination of the local distribution of interstellar NaI
Bibcode: 1998A&A...333..101W

Crifo, F.; Lallement, R.; Welsh, B. Y.

We present galactic maps of the distribution of neutral sodium absorption column density using the newly determined Hipparcos satellite distances for a total of 290 stars lying within 250pc of the Sun. These maps now replace those originally presented in Welsh {et al./} (1994). The Local Bubble is now seen to be a neutral gas-free cavity (nH<…

1998 Astronomy and Astrophysics
Hipparcos 35
NGC 2264 IRS: Evidence for Triggered Star Formation
DOI: 10.1086/311096 Bibcode: 1998ApJ...492L.177T

Schneider, Glenn; Thompson, Rodger I.; Corbin, Michael R. +1 more

As part of its commissioning process the Near-Infrared Camera and Multiobject Spectrometer (NICMOS) obtained images of the infrared source NGC 2264 IRS, also known as Allen's source, in three colors . In addition to the completely overexposed image of IRS there are six point objects, never previously observed, at projected separations of 2.6" to 4…

1998 The Astrophysical Journal
eHST 35