activity
19972001
most citedHST STIS Observations of PG 0946+301: the Highest Quality UV Spectrum of a BALQSO

127 citations · 200 across the 2 of their papers we have counts for

collaborators

7 papers

astro-ph2001★ 127 cited

HST STIS Observations of PG 0946+301: the Highest Quality UV Spectrum of a BALQSO

Nahum Arav, Martijn de Kool, Kirk T. Korista +16

We describe deep (40 orbits) HST/STIS observations of the BALQSO PG 0946+301 and make them available to the community. These observations are the major part of a multi-wavelength c…

astro-ph2001★ 73 cited

On the Column Density of AGN Outflows: the Case of NGC 5548

Nahum Arav, Martijn de Kool, Kirk T. Korista

We re-analyze the HST high resolution spectroscopic data of the intrinsic absorber in NGC 5548 and find that the C IV absorption column density is at least four times larger than p…

astro-ph2000

Keck Hires Observations of the QSO First J104459.6+365605: Evidence for a Large Scale Outflow

Martijn de Kool, Nahum Arav, Robert H. Becker +5

This paper presents an analysis of a Keck HIRES spectrum of the QSO FIRST J104459.6+365605. The line of sight towards the QSO contains two clusters of outflowing clouds that give r…

astro-ph1999

Thermal Instability and Evaporation of Accretion Disc Atmospheres

Martijn de Kool, Dayal T. Wickramasinghe

We investigate the thermal stability of the outer layers of accretion discs in which the local viscous energy dissipation rate scales with the pressure as for standard Shakura-Suny…

astro-ph1999

What Determines the Depth of BALs? Keck HIRES Observations of BALQSO 1603+300

Nahum Arav, Robert H. Becker, Sally A. Laurent-Muehleisen +3

We find that the depth and shape of the broad absorption lines (BALs) in BALQSO 1603+3002 are determined largely by the fraction of the emitting source which is covered by the BAL…

astro-ph1998

Accretion disk reversal and the spin-up/spin-down of accreting pulsars

James R. Murray, Martijn de Kool, Jianke Li

We numerically investigate the hydrodynamics of accretion disk reversal and relate our findings to the observed spin-rate changes in the accreting X-ray pulsar GX~1+4. In this syst…