Recurrent Symbiotic Nova V407 Cygni: Before and after Outburst in 2010

Abstract: We present the results of our UBV JHKLM photometric and spectroscopic observations of V407 Cyg obtained in 2003–2015. No fast brightness variations of V407 Cyg have been detected since its RS Oph-type outburst in 2010. Now the binary demonstrates a low-excitation emission spectrum with Hα weaker than the [N II] 6584 Å line. It is a typical spectrum on the way to the passive state.

Location
Deutsche Nationalbibliothek Frankfurt am Main
Extent
Online-Ressource
Language
Englisch

Bibliographic citation
Recurrent Symbiotic Nova V407 Cygni: Before and after Outburst in 2010 ; volume:24 ; number:4 ; year:2015 ; pages:353-359 ; extent:7
Open astronomy ; 24, Heft 4 (2015), 353-359 (gesamt 7)

Creator
Esipov, V. F.
Kolotilov, E. A.
Shenavrin, V. I.
Tarasova, T. N.
Tatarnikov, A. M.
Tatarnikova, A. A.

DOI
10.1515/astro-2017-0236
URN
urn:nbn:de:101:1-2405271651001.563566267280
Rights
Open Access; Der Zugriff auf das Objekt ist unbeschränkt möglich.
Last update
14.08.2025, 10:55 AM CEST

Data provider

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Associated

  • Esipov, V. F.
  • Kolotilov, E. A.
  • Shenavrin, V. I.
  • Tarasova, T. N.
  • Tatarnikov, A. M.
  • Tatarnikova, A. A.

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