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Evidence of the Evolved Nature of the B[e] Star MWC 137

The result's identifiers

  • Result code in IS VaVaI

    <a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A_____%2F15%3A00445025" target="_blank" >RIV/67985815:_____/15:00445025 - isvavai.cz</a>

  • Result on the web

    <a href="http://dx.doi.org/10.1088/0004-6256/149/1/13" target="_blank" >http://dx.doi.org/10.1088/0004-6256/149/1/13</a>

  • DOI - Digital Object Identifier

    <a href="http://dx.doi.org/10.1088/0004-6256/149/1/13" target="_blank" >10.1088/0004-6256/149/1/13</a>

Alternative languages

  • Result language

    angličtina

  • Original language name

    Evidence of the Evolved Nature of the B[e] Star MWC 137

  • Original language description

    Our goal is to clarify the evolutionary stage of this peculiar object, and to study the CO molecular component of its circumstellar medium. To this purpose, we modeled the CO molecular bands using high-resolution K-band spectra.We find that MWC137 is surrounded by a detached cool (T = 1900 +/- 100 K) and dense (N = (3 +/- 1) +/- 10(21) cm(-2)) ring of CO gas orbiting the star with a rotational velocity, projected to the line of sight, of 84 +/- 2 km s(-1). We also find that the molecular gas is enrichedin the isotope C-13, excluding the classification of the star as a Herbig Be. The observed isotopic abundance ratio (C-12/C-13 = 25 +/- 2) derived from our modeling is compatible with a proto-planetary nebula, main-sequence, or supergiant evolutionary phase. However, based on some observable characteristics of MWC137, we propose that the supergiant scenario seems to be the most plausible. Hence, we suggest that MWC137 could be in an extremely short-lived phase, evolving from a B[e] supe

  • Czech name

  • Czech description

Classification

  • Type

    J<sub>x</sub> - Unclassified - Peer-reviewed scientific article (Jimp, Jsc and Jost)

  • CEP classification

    BN - Astronomy and celestial mechanics, astrophysics

  • OECD FORD branch

Result continuities

  • Project

  • Continuities

    I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace

Others

  • Publication year

    2015

  • Confidentiality

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

Data specific for result type

  • Name of the periodical

    Astronomical Journal

  • ISSN

    0004-6256

  • e-ISSN

  • Volume of the periodical

    149

  • Issue of the periodical within the volume

    1

  • Country of publishing house

    US - UNITED STATES

  • Number of pages

    9

  • Pages from-to

    "13/1"-"13/9"

  • UT code for WoS article

    000347308300013

  • EID of the result in the Scopus database