Amanote Research

Amanote Research

  • Register
  • Sign In

Phase Lags and Coherence of X-Ray Variability in Black Hole Candidates

Monthly Notices of the Royal Astronomical Society- United Kingdom

doi 10.1093/mnras/280.1.227

Full Text

Abstract

Available in

Categories

AstrophysicsAstronomyPlanetary ScienceSpace

Date

May 1, 1996

Authors

M. A. NowakB. A. Vaughan

Publisher

Oxford University Press (OUP)


Related search

Modeling the Time Variability of Black Hole Candidates

Annals of the New York Academy of Sciences
GeneticsMolecular BiologyBiochemistryNeuroscienceHistoryPhilosophy of Science
1998English

Central Black Hole Masses in Active Galactic Nuclei Inferred From X‐Ray Variability

Astrophysical Journal
AstrophysicsAstronomyPlanetary ScienceSpace
1998English

X-Ray and Radio Variability of M31*, the Andromeda Galaxy Nuclear Supermassive Black Hole

Astrophysical Journal
AstrophysicsAstronomyPlanetary ScienceSpace
2010English

X-Ray Radio Correlation in Black Hole Sources

2007English

A Model for Optical/X-Ray Correlation in Black Hole X-Ray Binaries

2011English

An Accreting Millisecond Pulsar With Black Hole–like X‐Ray Variability: IGR J00291+5934

Astrophysical Journal
AstrophysicsAstronomyPlanetary ScienceSpace
2007English

Super-Eddington Accretion in Black Hole X-Ray Binaries

International Astronomical Union Colloquium
2004English

X-Ray Determination of the Black-Hole Mass in Cygnus X-1

Symposium - International Astronomical Union
1998English

Optical Photometry of Black-Hole Candidates

Symposium - International Astronomical Union
1996English

Amanote Research

Note-taking for researchers

Follow Amanote


© 2026 Amaplex Software S.P.R.L. All rights reserved.

Privacy PolicyRefund Policy