Titlebook: Disc Winds Matter; Modelling Accretion James Matthews Book 2017 Springer International Publishing AG 2017 Astrophysical Outflows.Accretion

使高兴

Space groups (189) P-62m – (174) P-6In the previous chapter, I presented tests of geometric unification models using MCRT and photoionization simulations.

Altitude

LATER

Introduction,The release of gravitational potential energy as mass falls towards a compact object is the most efficient energetic process in the universe, even more efficient than nuclear fusion.

政府

事与愿违

HEW

The Impact of Accretion Disc Winds on the Optical Spectra of Cataclysmic Variables,Here, I present Monte Carlo radiative transfer simulations designed to assess the likely impact of accretion disc winds on the optical spectra of high-state CVs.

Creatinine-Test

Testing Quasar Unification: Radiative Transfer in Clumpy Winds,In Chaps. . and ., I reviewed the observational evidence for accretion disc winds in quasars and luminous AGN, and showed how they may be responsible for more than just the broad absorption lines and P-Cygni profiles seen in quasar spectra.

mydriatic

Quasar Emission Lines as Probes of Orientation and Unification,In the previous chapter, I presented tests of geometric unification models using MCRT and photoionization simulations.

subordinate

regale