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CPD-64 degrees 2731: a massive spun-up and rejuvenated high-velocity runaway star

The result's identifiers

  • Result code in IS VaVaI

    <a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A_____%2F19%3A00511173" target="_blank" >RIV/67985815:_____/19:00511173 - isvavai.cz</a>

  • Result on the web

    <a href="https://doi.org/10.1093/mnras/sty2987" target="_blank" >https://doi.org/10.1093/mnras/sty2987</a>

  • DOI - Digital Object Identifier

    <a href="http://dx.doi.org/10.1093/mnras/sty2987" target="_blank" >10.1093/mnras/sty2987</a>

Alternative languages

  • Result language

    angličtina

  • Original language name

    CPD-64 degrees 2731: a massive spun-up and rejuvenated high-velocity runaway star

  • Original language description

    We report the results of our study of the high-velocity (approximate to 160 km s(-1)) runaway O star CPD-64 degrees 2731 and its associated horseshoe-shaped nebula discovered with the Wide-field Infrared Survey Explorer. Spectroscopic observations with the Southern African Large Telescope and spectral analysis indicate that CPD-64 degrees 2731 is a fast-rotating main-sequence O5.5 star with enhanced surface nitrogen abundance. We derive a projected rotational velocity of approximate to 300 km s(-1) that is extremely high for this spectral type. Its kinematic age of approximate to 6 Myr, assuming it was born near the Galactic plane, exceeds its age derived from single star models by a factor of 2. These properties suggest that CPD-64 degrees 2731 is a rejuvenated and spun-up binary product. The geometry of the nebula and the almost central location of the star within it argue against a pure bow shock interpretation for the nebula. Instead, we suggest that the binary interaction happened recently, thereby creating the nebula, with a cavity blown by the current fast stellar wind. This inference is supported by our results of 2D numerical hydrodynamic modelling.

  • Czech name

  • Czech description

Classification

  • Type

    J<sub>imp</sub> - Article in a specialist periodical, which is included in the Web of Science database

  • 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

    2019

  • Confidentiality

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

Data specific for result type

  • Name of the periodical

    Monthly Notices of the Royal Astronomical Society

  • ISSN

    1365-2966

  • e-ISSN

  • Volume of the periodical

    482

  • Issue of the periodical within the volume

    4

  • Country of publishing house

    GB - UNITED KINGDOM

  • Number of pages

    14

  • Pages from-to

    4408-4421

  • UT code for WoS article

    000462327300011

  • EID of the result in the Scopus database

    2-s2.0-85061102345