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Delta-slow solution to explain B supergiant stars' winds

The result's identifiers

  • Result code in IS VaVaI

    <a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A_____%2F14%3A00454643" target="_blank" >RIV/67985815:_____/14:00454643 - isvavai.cz</a>

  • Result on the web

    <a href="http://dx.doi.org/10.1017/S1743921314006401" target="_blank" >http://dx.doi.org/10.1017/S1743921314006401</a>

  • DOI - Digital Object Identifier

    <a href="http://dx.doi.org/10.1017/S1743921314006401" target="_blank" >10.1017/S1743921314006401</a>

Alternative languages

  • Result language

    angličtina

  • Original language name

    Delta-slow solution to explain B supergiant stars' winds

  • Original language description

    A new radiation-driven wind solution called δ-slow was found by Curé et al. (2011) and it predicts a mass-loss rate and terminal velocity slower than the fast solution (m-CAK, Pauldrach et al. 1986). In this work, we present our first synthetic spectra based on the δ-slow solution for the wind of B supergiant (BSG) stars. We use the output of our hydrodynamical code HYDWIND as input in the radiative transport code FASTWIND (Puls et al. 2005). In order to obtain stellar and wind parameters, we try to reproduce the observed Hα, Hβ, Hγ, Hδ, Hei 4471, Hei 6678 and Heii 4686 lines. The synthetic profiles obtained with the new hydrodynamical solutions are in good agreement with the observations and could give us clues about the parameters involved in the radiation force.

  • 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

    2014

  • Confidentiality

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

Data specific for result type

  • Article name in the collection

    New windows on massive stars: asteroseismology, interferometry, and spectropolarimetry

  • ISBN

    9781107078581

  • ISSN

    1743-9213

  • e-ISSN

  • Number of pages

    2

  • Pages from-to

    104-105

  • Publisher name

    Cambridge University Press

  • Place of publication

    Cambridge

  • Event location

    Geneva

  • Event date

    Jun 23, 2014

  • Type of event by nationality

    WRD - Celosvětová akce

  • UT code for WoS article

    000453211700022