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researcher

T. Kallman

18 papers hereh-index 241.7k citations62 works total

Matching runs newest-first, so older work may not be attached to this profile yet.

author position
  • middle author10
  • last author2

Across the 12 of 18 papers where every author was matched, so the position is known.

fields
  • astro-ph.HE11
  • astro-ph4
  • astro-ph.GA2
  • astro-ph.EP1
same name
  • T. Kallman — 127 papers, h 45
  • T. Kallman — 40 papers, h 15
  • T. Kallman — 9 papers, h 13
  • T. Kallman — 3 papers, h 5

Either other researchers who publish under this name, or the same person where the external sources have not merged their records.

identity via Semantic Scholar / OpenAlex

activity
20032023
most citedThe Accretion Disk Wind in the Black Hole GRS 1915+105

70 citations · 395 across the 18 of their papers we have counts for

collaborators
Showing astro-phShow all

4 papers · 1 filter

astro-ph2008★ 40 cited

An axisymmetric hydrodynamical model for the torus wind in AGN. II: X-ray excited funnel flow

A. Dorodnitsyn, T. Kallman, D. Proga

We have calculated a series of models of outflows from the obscuring torus in active galactic nuclei (AGN). Our modeling assumes that the inner face of a rotationally supported tor…

astro-ph2007★ 36 cited

The Variable Warm Absorber in Circinus X-1

N. S. Schulz, T. E. Kallman, D. K. Galloway +1

We observed Circinus X-1 twice during a newly reached low-flux phase near zero orbital phase using the High-Energy Transmission Grating Spectrometer (HETGS) onboard Chandra. In bot…

astro-ph2004★ 29 cited

Fe II Diagnostic Tools for Quasars

E. Verner, F. Bruhweiler, D. Verner +3

The enrichment of Fe, relative to alpha-elements such as O and Mg, represents a potential means to determine the age of quasars and probe the galaxy formation epoch. To explore how…

astro-ph2003★ 56 cited

Chandra Grating Spectroscopy of the X-ray Binary 4U 1700-37 in a Flaring State

B. Boroson, S. Vrtilek, T. Kallman +1

Chandra X-ray Observatory grating spectra of the supergiant X-ray Binary 4U 1700-37 reveal emission lines from hydrogen and helium-like S, Si, Mg, and Ne in the 4-13 A range. The s…

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Not affiliated with arXiv. Researcher data from Semantic Scholar (ODC-BY) and OpenAlex.