Effects of Preionization in Radiative Shocks. I. Self-consistent Models

Journal Article · Sat Apr 01 04:00:00 EDT 2017 · Astrophysical Journal, Supplement Series

DOI:https://doi.org/10.3847/1538-4365/AA6541· OSTI ID:22872812

Sutherland, Ralph S.; Dopita, Michael A. ^[1]

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1. Research School of Astronomy and Astrophysics, Australian National University, Cotter Road, Weston Creek, ACT 2611 (Australia)

In this paper we treat the preionization problem in shocks over the velocity range 10 < v {sub s} < 1500 km s{sup −1} in a self-consistent manner. We identify four distinct classes of solutions controlled by the value of the shock-precursor parameter, Ψ=Q/v{sub s}, where Q is the ionization parameter of the UV photons escaping upstream. This parameter determines both the temperature and the degree of ionization of the gas entering the shock. In increasing velocity, the shock solution regimes are cold neutral precursors (v {sub s} ≲ 40 km s{sup −1}), warm neutral precursors (40 ≲ v {sub s} ≲ 75 km s{sup −1}), warm partly ionized precursors (75 ≲ v {sub s} ≲ 120 km s{sup −1}), and fast shocks in which the preshock gas is in photoionization equilibrium and is fully ionized. The main effect of a magnetic field is to push these velocity ranges to higher values and to limit the postshock compression. In order to facilitate comparison with observations of shocks, we provide a number of convenient scaling relationships for parameters, such as postshock temperature, compression factors, cooling lengths, and Hβ and X-ray luminosity.

• OSTI ID: 22872812
• Journal Information: Astrophysical Journal, Supplement Series, Journal Name: Astrophysical Journal, Supplement Series Journal Issue: 2 Vol. 229; ISSN 0067-0049; ISSN APJSA2
• Country of Publication: United States
• Language: English

Related Subjects

79 ASTRONOMY AND ASTROPHYSICS
COOLING
LUMINOSITY
MAGNETIC FIELDS
PHOTOIONIZATION
PHOTONS
SCALING
ULTRAVIOLET RADIATION
VELOCITY
X RADIATION