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
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Czech description
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Classification
Type
J<sub>imp</sub> - Article in a specialist periodical, which is included in the Web of Science database
CEP classification
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OECD FORD branch
10308 - Astronomy (including astrophysics,space science)
Result continuities
Project
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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
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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