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Resolution and Kinematics of Molecular Gas Surrounding the Cloverleaf Quasar at Z = 2.6 Using the Gravitational Lens
DOI: 10.1086/310580 Bibcode: 1997ApJ...479L...9Y

Yun, M. S.; Blandford, R. D.; Scoville, N. Z. +1 more

Gravitational lenses have long been advertised as primitive telescopes, capable of magnifying cosmologically distant sources. In this Letter we present new, 0.9" resolution CO (7-6) observations of the z = 2.56 Cloverleaf quasar (H1413+117) and spatially resolved images. By modeling the gravitational lens, we infer a size scale of 0.3" (~1 kpc) fo…

1997 The Astrophysical Journal
eHST 38
Improved Evidence for a Black Hole in M32 from HST/FOS Spectra. I. Observations
DOI: 10.1086/304690 Bibcode: 1997ApJ...488..119V

van der Marel, Roeland P.; Rix, Hans-Walter; de Zeeuw, P. Tim

We have obtained spectra through small apertures centered on the nuclear region and major axis of M32 with the Faint Object Spectrograph (FOS) on the Hubble Space Telescope (HST). A detailed analysis and reduction of the data is presented, including (1) new calibrations and modeling of the FOS aperture sizes, point-spread function, and line-spread…

1997 The Astrophysical Journal
eHST 38
On the Origin of the Ultraviolet Continuum in Seyfert 2 Galaxies
DOI: 10.1086/310945 Bibcode: 1997ApJ...488L..71C

Colina, Luis; Pérez, Enrique; Mas-Hesse, J. Miguel +4 more

High-resolution Hubble Space Telescope ultraviolet images of the Seyfert 2 galaxies NGC 1667, NGC 3982, NGC 5427, and NGC 5953, previously known to have circumnuclear star-forming rings, are presented.

The UV images of all four Seyfert 2 galaxies show the presence of several compact UV-bright knots at distances of ~0.7-2 kpc from the nucleus …

1997 The Astrophysical Journal
eHST 38
Keck Spectroscopy of Objects with Lens-like Morphologies in the Hubble Deep Field
DOI: 10.1086/310416 Bibcode: 1997ApJ...474L...1Z

Zepf, Stephen E.; Davis, Marc; Moustakas, Leonidas A.

We present spectroscopy from the Keck telescope of three sets of objects in the Hubble Deep Field (HDF) that have lens-like morphologies. In the case of J123641+621204, which is composed of four objects with similar colors and a mean separation of <~0.8", we find at least two distinct components at redshifts of z = 3.209 and z = 3.220 that are …

1997 The Astrophysical Journal
eHST 38
Radio Emission from Objects in the Hubble Deep Field
DOI: 10.1086/310457 Bibcode: 1997ApJ...475L...5F

Fomalont, E. B.; Windhorst, R. A.; Richards, E. A. +2 more

A radio image that covers the Hubble deep field and flanking fields has been made using the VLA for 50 hr at a frequency of 8.4 GHz, a resolution of 6", and a 4.3 σ detection level of 12.2 µJy. All six radio sources detected in the deep field are identified with galaxies brighter than I = 24 mag, based on a radio/optical coincidence better t…

1997 The Astrophysical Journal
eHST 38
Modeling the distribution of magnetic fluxes in field concentrations in a solar active region
DOI: 10.1023/A:1004901916229 Bibcode: 1997SoPh..175..329S

Shine, Richard A.; Title, Alan M.; Schrijver, Carolus J. +1 more

Much of the magnetic field in solar and stellar photospheres is arranged into clusters of `flux tubes', i.e., clustered into compact areas in which the intrinsic field strength is approximately a kilogauss. The flux concentrations are constantly evolving as they merge with or annihilate against other concentrations, or fragment into smaller concen…

1997 Solar Physics
SOHO 37
Observations of the Hubble Deep Field with the Infrared Space Observatory - II. Source detection and photometry
DOI: 10.1093/mnras/289.2.465 Bibcode: 1997MNRAS.289..465G

Elbaz, D.; Danese, L.; Franceschini, A. +18 more

We present positions and fluxes of point sources found in the Infrared Space Observatory (ISO) images of the Hubble Deep Field (HDF) at 6.7 and 15 mu. We have constructed algorithmically selected `complete' flux-limited samples of 19 sources in the 15-mu image, and seven sources in the 6.7-mu image. The typical flux limit at 15 mu is ~0.2 mJy and …

1997 Monthly Notices of the Royal Astronomical Society
ISO 37
Rings and Satellites of Uranus: Colorful and Not So Dark
DOI: 10.1006/icar.1996.5631 Bibcode: 1997Icar..125..348K

Karkoschka, Erich

Photometric properties of nine uranian satellites and four rings, based on six Hubble Space Telescope images taken in 1995, are presented. Derived albedos are consistent with previous data taken at the same phase angle of 1°, but inconsistent with most Voyager-based estimates extrapolated from observations at phase angles above 15°. The shape of p…

1997 Icarus
eHST 37
The Digital Wave-Processing Experiment on Cluster
DOI: 10.1023/A:1004914211866 Bibcode: 1997SSRv...79..209W

Woolliscroft, L. J. C.; Alleyne, H. St. C.; Dunford, C. M. +7 more

1997 Space Science Reviews
Cluster 37
Hubble Space Telescope Beryllium Abundances in the α Centauri System
DOI: 10.1086/304004 Bibcode: 1997ApJ...480..784P

Pinsonneault, M. H.; Deliyannis, Constantine P.; Primas, F. +2 more

High signal-to-noise ratio Hubble Space Telescope Goddard High-Resolution Spectrograph spectra of α Centauri A (spectral type G2 V) and α Centauri B (spectral type K1 V) have been analyzed in the Be II λ3130 spectral region. Both stars offer an excellent opportunity for testing predictions of 9Be destruction since they are nearby, have …

1997 The Astrophysical Journal
eHST 37