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

使高興

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

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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.

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事與愿違

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.

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regale