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
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Czech description
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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
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Result continuities
Project
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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
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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
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