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Evidence for Galaxy Interactions/Mergers from Medium Deep Survey WFPC2 Data
DOI: 10.1086/303937 Bibcode: 1997ApJ...480...59N

Im, M.; Griffiths, R. E.; Ratnatunga, K. U. +3 more

We examine the morphological and statistical properties of close galaxy pairs from two sets of 28 WFPC2 fields, acquired for the Medium Deep Survey (MDS) and the Groth-Westphal Survey (GWS) in F606W (V) and F814W (I) passbands. In the GWS sample all fields have uniform 95% completeness down to I <~ 24.3 mag, whereas in the MDS sample, fields ha…

1997 The Astrophysical Journal
eHST 48
The Distance to the Coma Cluster from Surface Brightness Fluctuations
DOI: 10.1086/310735 Bibcode: 1997ApJ...483L..37T

Baum, William A.; Hammergren, Mark; Thomsen, Bjarne +1 more

We report on the first determination of the distance to the Coma Cluster from surface brightness fluctuation (SBF) measurements obtained from Hubble Space Telescope WFPC2 observations of the bright E0 galaxy NGC 4881 in the Coma Cluster and ground-based observations of the ``standard'' E1 galaxy NGC 3379 in the Leo-I group. Relative distances base…

1997 The Astrophysical Journal
eHST 47
Imaging the nuclear environment of NGC 1365 with the Hubble Space Telescope
Bibcode: 1997A&A...328..483K

Boksenberg, Alec; Lindblad, Per Olof; Kristen, Helmuth +1 more

The region surrounding the active nucleus of the barred spiral galaxy NGC 1365 is observed in the [Oiii] lambda 5007 line and neighbouring continuum using the Faint Object Camera (FOC) aboard the Hubble Space Telescope (HST). In the continuum light numerous bright ``super star clusters'' (SSCs) are seen in the nuclear region. They tend to fall on …

1997 Astronomy and Astrophysics
eHST 47
Detection of SO2 on Callisto with the Hubble Space Telescope
DOI: 10.1029/97GL00876 Bibcode: 1997GeoRL..24.1139N

Johnson, Robert E.; McGrath, Melissa A.; Noll, Keith S. +1 more

We have detected SO2 in ultraviolet spectra of Callisto obtained with the Hubble Space Telescope's Faint Object Spectrograph. An absorption band centered at 280 nm appears in the spectrum of Callisto's leading hemisphere, but is not apparent in the spectrum of the trailing hemisphere. The band is similar to the SO2 band on Eu…

1997 Geophysical Research Letters
eHST 47
A 200km/s molecular wind in the peculiar carbon star V Hya.
Bibcode: 1997A&A...326..318K

Jorissen, A.; Knapp, G. R.; Young, K.

A molecular wind with an outflow speed in excess of 200km/s has been found in the AGB carbon star V Hya. Observations of several molecular lines show that the circumstellar envelope is expanding at 15km/s and is flattened and inclined to the line of sight. The fast wind appears to be expanding from the poles of the envelope, with the expansion spe…

1997 Astronomy and Astrophysics
IUE 47
The Discovery of Mg II λ4481 in the White Dwarf EG 102: Evidence for Ongoing Accretion
DOI: 10.1086/310446 Bibcode: 1997ApJ...474L.127H

Barstow, M. A.; Holberg, J. B.; Green, Elizabeth M.

Recent optical spectra of the DA3 white dwarf EG 102 clearly show a feature due to Mg II λ4481. This is the first spectroscopic detection of Mg in a DA star at a temperature of 20,000 K. The presence of this ion in the stellar photosphere poses a severe dilemma for the theory of radiative levitation, which predicts a vanishingly small equilibrium …

1997 The Astrophysical Journal
IUE 47
The Pele Plume (Io): Observations with the Hubble Space Telescope
DOI: 10.1029/97GL02592 Bibcode: 1997GeoRL..24.2471S

Ballester, Gilda E.; McGrath, Melissa A.; Spencer, John R. +3 more

In July 1996, with the Hubble Space Telescope (HST), we observed the Pele plume silhouetted against Jupiter at a wavelength of 0.27µm, the first definitive observation of an Io plume from Earth. The height, 420 ± 40 km, was greater than any plume observed by Voyager. The plume had significantly smaller optical depth at 0.34 and 0.41µm, where it wa…

1997 Geophysical Research Letters
eHST 47
Hubble Space Telescope Spectrum of SN 1987A at an Age of 8 Years: Radioactive Luminescence of Cool Gas
DOI: 10.1086/304253 Bibcode: 1997ApJ...483..925C

Challis, Peter M.; Chevalier, Roger A.; Kirshner, Robert P. +1 more

The Hubble Space Telescope 2000-8000 Å spectrum of SN 1987A observed on 1995 January 7 (7.87 yr after the explosion) is dominated by Hα and UV lines, including Mg II-Mg I λ2825 (equal to Hα in luminosity), Fe II UV 2 (two-thirds the intensity of Hα), Fe II UV 3 (one-half the intensity of Hα), and a 3730 Å emission feature identified with a blend o…

1997 The Astrophysical Journal
eHST 47
High Velocity Features in the Orion Nebula
DOI: 10.1086/118622 Bibcode: 1997AJ....114.2016O

Hartigan, Patrick; O'Dell, C. R.; Bally, John +1 more

We have surveyed the inner 7' of the Orion Nebula for high velocity outflows with Fabry-Perot images in [S II] and [O III]. The new survey recovers all known HH objects in the region, and also reveals a number of new high velocity flows. New flows include (1) jets over an arcminute in length that extend from the center of the nebula to HH 202 in t…

1997 The Astronomical Journal
eHST 47
Spectroscopy of Close Companions to Quasi-Stellar Objects and the Ages of Interaction-Induced Starbursts
DOI: 10.1086/310608 Bibcode: 1997ApJ...480L...5C

Stockton, Alan; Canalizo, Gabriela

We present low-resolution absorption-line spectra of three candidate close (<3") companions to the low-redshift QSOs 3CR 323.1, PG 1700+518, and PKS 2135-147. The spectra were obtained with the Low-Resolution Imaging Spectrometer (LRIS) on the Keck telescopes and with the Faint Object Spectrograph on the University of Hawaii 2.2 m telescope. Fo…

1997 The Astrophysical Journal
eHST 46