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Light curve modeling for time-dependent accretion disks in X-ray novae with general relativity effects taken into account
Suleimanov V., Lipunova G., Shakura N.
-disks in X-ray novae. The model is based on an analytic solution for α-disk evolution after the outburst
Constraining the role of novae as progenitors of type Ia supernovae
Soraisam M., Gilfanov M.
, various types of accreting white dwarfs (WDs) have been proposed as prospective candidates. One
Modeling of non-stationary accretion disks in X-ray novae A 0620-00 and GRS 1124-68 during outburst
Suleimanov F., Lipunova V., Shakura I.
Aims. We address the task of modeling soft X-ray and optical light curves of X-ray novae
Light curve modeling for time-dependent accretion disks in X-ray novae with general relativity effects taken into account
Suleimanov V., Lipunova G., Shakura N.
-disks in X-ray novae. The model is based on an analytic solution for α-disk evolution after the outburst
Modelling nova populations in galaxies
Chen H., Woods T., Yungelson L., Gilfanov M., Han Z.
© 2016 The Authors.Theoretical modelling of the evolution of classical and recurrent novae plays
Constraining the role of novae as progenitors of type Ia supernovae
Soraisam M., Gilfanov M.
, various types of accreting white dwarfs (WDs) have been proposed as prospective candidates. One
Modeling of non-stationary accretion disks in X-ray novae A 0620-00 and GRS 1124-68 during outburst
Suleimanov F., Lipunova V., Shakura I.
Aims. We address the task of modeling soft X-ray and optical light curves of X-ray novae
Modelling nova populations in galaxies
Chen H., Woods T., Yungelson L., Gilfanov M., Han Z.
© 2016 The Authors.Theoretical modelling of the evolution of classical and recurrent novae plays
Optical observations of 'hot' novae returning to quiescence
© 2018 The Author(s). We have monitored the return to quiescence of novae previously observed
OT J002656.6+284933 (CSS101212:002657+284933): An SU UMa-type dwarf nova with the longest superhump period
Kato T., Tordai T., Littlefield C., Kasai K., Shugarov S., Katysheva N., Zaostrojnykh A., Pickard R., De Miguel E., Antonyuk K., Antonyuk O., Pavlenko E., Pit N., Itoh H., Ruiz J., Isogai K., Kimura M., Wakamatsu Y., Vanmunster T., Stone G.
] superhumps among SU UMa-type dwarf novae. The object is the third known SU UMa-type dwarf nova above

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