A Super-Eddington Wind Model for GRO J1655–40

International Astronomical Union Colloquium
doi 10.1017/s0252921100042512
Full Text
Abstract

Available in full text

Date
Authors
Publisher

Cambridge University Press (CUP)

Related search

The Radio Surroundings of the Microquasar GRO J1655-40

Astronomy and Astrophysics
AstrophysicsAstronomyPlanetary ScienceSpace
2001English

The Black Hole Binary Nova Scorpii 1994 (GRO J1655-40): An Improved Chemical Analysis

Astronomy and Astrophysics
AstrophysicsAstronomyPlanetary ScienceSpace
2009English

Microlensing Evidence for Super-Eddington Disk Accretion in Quasars

Proceedings of the International Astronomical Union
AstrophysicsAstronomyPlanetary ScienceSpace
2012English

Are Quasars Accreting at Super-Eddington Rates?

Astronomy and Astrophysics
AstrophysicsAstronomyPlanetary ScienceSpace
2002English

Super-Eddington Wind Scenario for the Progenitors of Type Ia Supernovae: Accreting He-Rich Matter Onto White Dwarfs

Astronomy and Astrophysics
AstrophysicsAstronomyPlanetary ScienceSpace
2015English

V4641Sgr – A Super-Eddington Source Enshrouded by an Extended Envelope

Astronomy and Astrophysics
AstrophysicsAstronomyPlanetary ScienceSpace
2002English

Super-Eddington Accretion in Black Hole X-Ray Binaries

International Astronomical Union Colloquium
2004English

A Modeling of the Super-Eddington Luminosity in Nova Outbursts: V1974 Cygni

Astrophysical Journal
AstrophysicsAstronomyPlanetary ScienceSpace
2005English

GRO J1008 57: A Laboratory for Accretion Physics

2013English

Amanote Research

Note-taking for researchers

Follow Amanote

© 2024 Amaplex Software S.P.R.L. All rights reserved.

Privacy PolicyRefund Policy