5
views
0
recommends
+1 Recommend
0 collections
    0
    shares
      • Record: found
      • Abstract: not found
      • Article: not found

      The disc instability model for X-ray transients: Evidence for truncation and irradiation

      , ,
      Astronomy & Astrophysics
      EDP Sciences

      Read this article at

      ScienceOpenPublisher
      Bookmark
          There is no author summary for this article yet. Authors can add summaries to their articles on ScienceOpen to make them more accessible to a non-specialist audience.

          Related collections

          Most cited references45

          • Record: found
          • Abstract: not found
          • Article: not found

          Advection‐Dominated Accretion and the Spectral States of Black Hole X‐Ray Binaries: Application to Nova Muscae 1991

            Bookmark
            • Record: found
            • Abstract: not found
            • Article: not found

            The disc instability model of dwarf novae and low-mass X-ray binary transients

              Bookmark
              • Record: found
              • Abstract: not found
              • Article: not found

              The Properties of X‐Ray and Optical Light Curves of X‐Ray Novae

                Bookmark

                Author and article information

                Journal
                Astronomy & Astrophysics
                A&A
                EDP Sciences
                0004-6361
                1432-0746
                July 2001
                July 15 2001
                July 2001
                : 373
                : 1
                : 251-271
                Article
                10.1051/0004-6361:20010632
                ec02d976-4367-4502-b179-b87af83a751f
                © 2001
                History

                Comments

                Comment on this article