Coordinated integral and optical observations of SS433Cherepashchuk A.,
Sunyaev R.,
Fabrikat S.,
Molkov S.,
Barsukova E.,
Antokhina E.,
Irsmambetova T.,
Panchenko I.,
Postnov K.,
Seifina E.,
Shakura N.,
Timokhin A.,
Bikmaev I.,
Sakhibullin N.,
Gnedin Y.,
Arkharov A.,
Larionov V. is discovered spectroscopically. The observed broadband X-ray spectrum 2-100 ke
V can be described by emission
Photometry and spectroscopy of the luminous red nova PSNJ14021678+5426205 in the galaxy M101Goranskij V.,
Barsukova E.,
Spiridonova O.,
Valeev A.,
Fatkhullin T.,
Moskvitin A.,
Vozyakova O.,
Cheryasov D.,
Safonov B.,
Zharova A.,
Hancock T. of the progenitor gradually increased by (Formula presented.) in the
V-band. At the peak of the first outburst
Coordinated integral and optical observations of SS433Cherepashchuk A.,
Sunyaev R.,
Fabrikat S.,
Molkov S.,
Barsukova E.,
Antokhina E.,
Irsmambetova T.,
Panchenko I.,
Postnov K.,
Seifina E.,
Shakura N.,
Timokhin A.,
Bikmaev I.,
Sakhibullin N.,
Gnedin Y.,
Arkharov A.,
Larionov V. is discovered spectroscopically. The observed broadband X-ray spectrum 2-100 ke
V can be described by emission
Progenitor and Remnant of the Luminous Red Nova V838 Monocerotis photometry, medium and low resolution spectroscopy of the red nova
V838 Mon remnant for 16 years after