Synthetic X-ray spectra for simulations of the dynamics of an accretion flow irradiated by a quasar-Reference-Cited by-同舟云学术

Synthetic X-ray spectra for simulations of the dynamics of an accretion flow irradiated by a quasar

Author:

Sim S. A.¹,Proga D.,Kurosawa R.²,Long K. S.³,Miller L.⁴,Turner T. J.⁵

Affiliation:

1. Research School of Astronomy and Astrophysics; Mount Stromlo Observatory; Cotter Road; Weston Creek; ACT; 2611; Australia

2. Department of Astronomy; Cornell University; Space Sciences Building; Ithaca; NY; 14853-6801; USA

3. Space Telescope Science Institute; 3700 San Martin Drive; Baltimore; MD; 21218; USA

4. Department of Physics; University of Oxford; Denys Wilkinson Building, Keble Road; Oxford; OX1 3RH

5. Department of Physics; University of Maryland Baltimore County; 1000 Hilltop Circle; Baltimore; MD; 21250; USA

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

Reference48 articles.

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