All

What are you looking for?

All
Projects
Results
Organizations

Quick search

  • Projects supported by TA ČR
  • Excellent projects
  • Projects with the highest public support
  • Current projects

Smart search

  • That is how I find a specific +word
  • That is how I leave the -word out of the results
  • “That is how I can find the whole phrase”

Wray 15-906 low mass Luminous Blue Variable in a pre-supernova stage

The result's identifiers

  • Result code in IS VaVaI

    <a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A_____%2F24%3A00646242" target="_blank" >RIV/67985815:_____/24:00646242 - isvavai.cz</a>

  • Result on the web

    <a href="http://dx.doi.org/10.1017/S1743921322002733" target="_blank" >http://dx.doi.org/10.1017/S1743921322002733</a>

  • DOI - Digital Object Identifier

    <a href="http://dx.doi.org/10.1017/S1743921322002733" target="_blank" >10.1017/S1743921322002733</a>

Alternative languages

  • Result language

    angličtina

  • Original language name

    Wray 15-906 low mass Luminous Blue Variable in a pre-supernova stage

  • Original language description

    The evolutionary link between Red Supergiants and Luminous Blue variables is interesting, but still poorly understood. We present the results of a study of the Galactic candidate luminous blue variable Wray 15-906, revealed via the detection of its infrared circumstellar shell (of ≍2 pc in diameter) with the Wide-field Infrared Survey Explorer (WISE) and the Herschel Space Observatory. Using the stellar atmosphere code CMFGEN and the Gaia parallax, we found that Wray 15-906 is a relatively low-luminosity, log(L/Lȯ) ≍ 5.4, star with a temperature of 25±2 kK. In the framework of single star evolution, the obtained results suggest that Wray 15-906 is a post-red supergiant star with an initial mass of ≍ 25Mȯ and that before exploding as a supernova it could transform for a short time into a WN11h star. The presence of a shell with a mass 2.9±0.5Me indicates that Wray 15-906 has suffered substantial mass loss in the recent past.

  • Czech name

  • Czech description

Classification

  • Type

    D - Article in proceedings

  • CEP classification

  • OECD FORD branch

    10308 - Astronomy (including astrophysics,space science)

Result continuities

  • Project

  • Continuities

    I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace

Others

  • Publication year

    2024

  • Confidentiality

    S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

Data specific for result type

  • Article name in the collection

    Proceedings of the International Astronomical Union

  • ISBN

  • ISSN

    1743-9213

  • e-ISSN

    1743-9221

  • Number of pages

    2

  • Pages from-to

    460-461

  • Publisher name

    Cambridge University Press

  • Place of publication

    Cambridge

  • Event location

    Ballyconnell

  • Event date

    May 8, 2022

  • Type of event by nationality

    WRD - Celosvětová akce

  • UT code for WoS article