The Correlation Between Hard X-Ray Peak Flux and Soft X-Ray Peak Flux in the Outburst Rise of Low-Mass X-Ray Binaries

Astrophysical Journal - United States
doi 10.1086/423953
Full Text
Abstract

Available in full text

Date
Authors
Publisher

IOP Publishing

Related search

Hard X‐Ray Emission From Low‐Mass X‐Ray Binaries

Astrophysical Journal
AstrophysicsAstronomyPlanetary ScienceSpace
2000English

Hard X-Ray Emission From Low Mass X-Ray Binaries

Chinese Journal of Astronomy and Astrophysics
2003English

Low-Mass X-Ray Binaries as the Source of the Very Soft X-Ray Emission in the X-Ray–faintest Early-Type Galaxies

Astrophysical Journal
AstrophysicsAstronomyPlanetary ScienceSpace
1998English

Low-Mass X-Ray Binaries and Their Relation to the Non-X-Ray Sources

Annals of the New York Academy of Sciences
GeneticsMolecular BiologyBiochemistryNeuroscienceHistoryPhilosophy of Science
1977English

Low-Mass X-Ray Binaries—Recent Developments

1996English

Recycled Pulsars and Low Mass X-Ray Binaries

International Astronomical Union Colloquium
1992English

The Discovery of an Outburst and Pulsed X-Ray Flux From SMC X-2 Using the [ITAL]Rossi X-Ray Timing Explorer[/Ital]

Astrophysical Journal
AstrophysicsAstronomyPlanetary ScienceSpace
2001English

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

2011English

The Radio and X-Ray Correlation in a Sample of Hard X-Ray Selected AGN

2012English

Amanote Research

Note-taking for researchers

Follow Amanote

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

Privacy PolicyRefund Policy