Search Publications

Optical-IUE observations of the gamma-ray loud BL Lacertae object S5 0716+714: data and interpretation.
DOI: 10.48550/arXiv.astro-ph/9706254 Bibcode: 1997A&A...327...61G

Maraschi, L.; Ghisellini, G.; Pian, E. +14 more

We monitored the BL Lac object S5 0716+714 in the optical band during the period November 1994 - April 1995, which includes the time of a γ-ray observation by the Energetic Gamma Ray Experiment Telescope (EGRET) on February 14-28, 1995. The light curves in the R and B bands show fast fluctuations superimposed on longer timescale variations. The co…

1997 Astronomy and Astrophysics
IUE 183
Absolute Magnitude Calibration for the W UMa-Type Systems Based on HIPPARCOS Data
DOI: 10.1086/134014 Bibcode: 1997PASP..109.1340R

Rucinski, S. M.; Duerbeck, H. W.

Hipparcos parallax data for 40 contact binary stars of the W UMa-type (with epsilon M_V < 0.5) are used to derive a new, (B-V)-based absolute-magnitude calibration of the form M_V = M_V(log P,B-V). The calibration covers the ranges 0.26 < (B-V)_0 < 1.14, 0.24 < P < 1.15 day, and 1.4 < M_V < 6.1; it is based on a solution weigh…

1997 Publications of the Astronomical Society of the Pacific
Hipparcos 183
Optical Rotation Curves of Distant Field Galaxies: Sub-L* Systems
DOI: 10.1086/310591 Bibcode: 1997ApJ...479L.121V

Illingworth, Garth D.; Faber, S. M.; Gronwall, Caryl +6 more

Moderate-resolution spectroscopic observations from the Keck 10 m telescope are used to derive internal kinematics for eight faint disk galaxies in the fields flanking the Hubble Deep Field. The spectroscopic data are combined with high-resolution F814W Wide Field Planetary Camera 2 images from the Hubble Space Telescope that provide morphologies,…

1997 The Astrophysical Journal
eHST 182
Ellipticals with Kinematically Distinct Cores: V - I Color Images with WPFC2
DOI: 10.1086/304060 Bibcode: 1997ApJ...481..710C

Franx, Marijn; Illingworth, Garth D.; Forbes, Duncan A. +1 more

We have analyzed Hubble Space Telescope WFPC2 F555W and F814W (i.e., V and I) images for 15 elliptical galaxies with kinematically distinct cores. For each of them, we have derived surface brightness and isophotal parameter profiles in the two bands, color maps, and radial profiles in V - I. Most galaxies show patchy dust absorption close to their…

1997 The Astrophysical Journal
eHST 182
HST observations of blue Straggler stars in the core of the globular cluster M 3.
DOI: 10.48550/arXiv.astro-ph/9703026 Bibcode: 1997A&A...324..915F

Burgarella, D.; Cacciari, C.; Buonanno, R. +7 more

The core of the Galactic Globular Cluster M 3 (NGC 5272) has been observed with the WFPC2 through the filters F255W, F336W, F555W, and F814W. Using these observations along with a thorough reanalysis of earlier catalogs, we have produced a catalog of blue straggler stars (BSS) spanning the cluster. Earlier studies and the fainter part of our sampl…

1997 Astronomy and Astrophysics
eHST 180
The optical counterpart to γ-ray burst GRB970228 observed using the Hubble Space Telescope
DOI: 10.1038/387476a0 Bibcode: 1997Natur.387..476S

Livio, Mario; Kouveliotou, Chryssa; Sahu, Kailash C. +7 more

Although more than 2,000 astronomical γ-ray bursts (GRBs) have been detected, and numerous models proposed to explain their occurrence1, they have remained enigmatic owing to the lack of an obvious counterpart at other wavelengths2-5. The recent ground-based detection6,7 of a transient optical source in the vicinit…

1997 Nature
eHST 176
An Empirical Study of the Electron Temperature and Heavy Ion Velocities in the South Polar Coronal Hole
DOI: 10.1023/A:1004943213433 Bibcode: 1997SoPh..171..345K

Gloeckler, George; Geiss, Johannes; Fisk, Lennard A. +2 more

The solar wind ions flowing outward through the solar corona generally have their ionic fractions `freeze-in' within 5 solar radii. The altitude where the freeze-in occurs depends on the competition between two time scales: the time over which the wind flows through a density scale height, and the time over which the ions achieve ionization equili…

1997 Solar Physics
Ulysses 174
Steps toward Determination of the Size and Structure of the Broad-Line Region in Active Galactic Nuclei. XI. Intensive Monitoring of the Ultraviolet Spectrum of NGC 7469
DOI: 10.1086/313054 Bibcode: 1997ApJS..113...69W

Shull, J. M.; Malkan, M. A.; Nandra, K. +54 more

From 1996 June 10 to July 29, the International Ultraviolet Explorer monitored the Seyfert 1 galaxy NGC 7469 continuously in an attempt to measure time delays between the continuum and emission-line fluxes. From the time delays, one can estimate the size of the region dominating the production of the UV emission lines in this source. We find the s…

1997 The Astrophysical Journal Supplement Series
IUE 174
Patchy intergalactic He II absorption in HE 2347-4342. II. The possible discovery of the epoch of He-reionization
DOI: 10.48550/arXiv.astro-ph/9707173 Bibcode: 1997A&A...327..890R

Reimers, D.; Wamsteker, W.; Rodriguez-Pascual, P. +3 more

We report on observations of redshifted Heii303.8 Angstroms absorption in the high-redshift QSO HE2347-4342 (z=2.885, V=16.1) with the Goddard High Resolution Spectrograph on board HST in its low resolution mode (bigtriangleup lambda = 0.7 Angstroms). With f_λ=3.6\ 10(-15) ergcm(-2) s(-1) Angstroms(-1) at the expected position of Heii304 Angstroms…

1997 Astronomy and Astrophysics
IUE eHST 169
The Ultraviolet Properties of the Narrow-Line Quasar I Zw 1
DOI: 10.1086/304816 Bibcode: 1997ApJ...489..656L

Laor, Ari; Green, Richard F.; Jannuzi, Buell T. +1 more

I Zwicky 1 (I Zw 1) is the prototype narrow-line quasar. Its narrow-line profiles minimize blending effects and thus allow a significantly more accurate study of individual quasar emission lines. We report here the results of our study of the 1150-3250 Å emission of I Zw 1 using a high signal-to-noise (50-120) spectrum obtained with the Faint Obje…

1997 The Astrophysical Journal
eHST 168