Amanote Research

Amanote Research

    RegisterSign In

X-Ray Emission From Supermassive Black Holes in Elliptical Galaxies and Low Radiative-Efficiency Accretion

Symposium - International Astronomical Union
doi 10.1017/s0074180900163211
Full Text
Open PDF
Abstract

Available in full text

Date

January 1, 2000

Authors
T. Di MatteoS. W. Allen
Publisher

Cambridge University Press (CUP)


Related search

The Brightest Point X‐Ray Sources in Elliptical Galaxies and the Mass Spectrum of Accreting Black Holes

Astrophysical Journal
AstrophysicsAstronomyPlanetary ScienceSpace
2006English

Spin Orientation of Supermassive Black Holes in Active Galaxies

Astronomy and Astrophysics
AstrophysicsAstronomyPlanetary ScienceSpace
2003English

Non-Quiescent X-Ray Emission From Neutron Stars and Black Holes

2003English

Coevolution of Supermassive Black Holes and Their Host Galaxies

AIP Conference Proceedings
AstronomyPhysics
2008English

X-Ray Heated Accretion Discs Around Stellar Mass Black Holes

International Astronomical Union Colloquium
2004English

Co-Evolution of Supermassive Black Holes and Their Host Galaxies

Proceedings of the International Astronomical Union
AstrophysicsAstronomyPlanetary ScienceSpace
2009English

Strong Soft X-Ray Emission and High Accretion Rates in Seyfert Galaxies

International Astronomical Union Colloquium
1997English

Searching for Low-Mass Supermassive Black Holes

Symposium - International Astronomical Union
1999English

X-Ray Emission From Hot Accretion Flows

Proceedings of the International Astronomical Union
AstrophysicsAstronomyPlanetary ScienceSpace
2013English

Amanote Research

Note-taking for researchers

Follow Amanote

© 2025 Amaplex Software S.P.R.L. All rights reserved.

Privacy PolicyRefund Policy