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19932004
most citedDust and Diffuse Interstellar Bands in the z_a = 0.524 Absorption System toward AO 0235+164

120 citations · 350 across the 12 of their papers we have counts for

collaborators

12 papers

astro-ph2004★ 120 cited

Dust and Diffuse Interstellar Bands in the z_a = 0.524 Absorption System toward AO 0235+164

V. T. Junkkarinen, Ross D. Cohen, E. A. Beaver +3

We present new HST STIS NUV-MAMA and STIS CCD observations of the BL Lac object AO 0235+164 and the intervening damped Ly alpha (DLA) line at z_a = 0.524. The line profile gives N(…

astro-ph2003★ 84 cited

Variability Tests for Intrinsic Absorption Lines in Quasar Spectra

Desika Narayanan, Fred Hamann, Tom Barlow +4

Quasar spectra have a variety of absorption lines whose origins range from energetic winds expelled from the central engines to unrelated, intergalactic clouds. We present multi-ep…

astro-ph2001★ 10 cited

UV Imaging Polarimetry of the peculiar Seyfert 2 galaxy Mrk 477

Makoto Kishimoto, Laura E. Kay, Robert Antonucci +3

We present the results of UV imaging polarimetry of the Seyfert 2 galaxy Mrk 477 taken by the Faint Object Camera onboard the Hubble Space Telescope (HST). From a previous HST UV i…

astro-ph2001★ 25 cited

UV Imaging Polarimetry of the Seyfert 2 Galaxy Mrk 3

Makoto Kishimoto, Laura E. Kay, Robert Antonucci +3

We present UV imaging polarimetry data of the Seyfert 2 galaxy Mrk 3 taken by the Hubble Space Telescope. The polarized flux is found to be extended to ~1 kpc from the nucleus, and…

astro-ph2001

HST UV and Keck HIRES Spectra of BAL Quasars

V. Junkkarinen, R. D. Cohen, T. A. Barlow +1

In the analysis of broad absorption line (BAL) quasar spectra, Keck HIRES spectra are a useful complement to lower resolution HST and ground based spectra. The HIRES spectra provid…

astro-ph2001

Discovery of a 2 Kpc Binary Quasar

G. A. Shields, V. Junkkarinen, E. A. Beaver +4

LBQS 01032753 is a binary quasar with a separation of only 0.3 arcsec. The projected spacing of 2.3 kpc at the distance of the source (z = 0.848) is much smaller than that of an…