A characteristic oxygen abundance gradient in galaxy disks unveiled with CALIFA
The result's identifiers
Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A_____%2F14%3A00429531" target="_blank" >RIV/67985815:_____/14:00429531 - isvavai.cz</a>
Result on the web
<a href="http://dx.doi.org/10.1051/0004-6361/201322343" target="_blank" >http://dx.doi.org/10.1051/0004-6361/201322343</a>
DOI - Digital Object Identifier
<a href="http://dx.doi.org/10.1051/0004-6361/201322343" target="_blank" >10.1051/0004-6361/201322343</a>
Alternative languages
Result language
angličtina
Original language name
A characteristic oxygen abundance gradient in galaxy disks unveiled with CALIFA
Original language description
We present the largest and most homogeneous catalog of H II regions and associations compiled so far. The catalog comprises more than 7000 ionized regions, extracted from 306 galaxies observed by the CALIFA survey. We describe the procedures used to detect, select, and analyze the spectroscopic properties of these ionized regions. In the current study we focus on characterizing of the radial gradient of the oxygen abundance in the ionized gas, based on the study of the deprojected distribution of H II regions.
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
2014
Confidentiality
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů
Data specific for result type
Name of the periodical
Astronomy & Astrophysics
ISSN
0004-6361
e-ISSN
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Volume of the periodical
563
Issue of the periodical within the volume
March
Country of publishing house
FR - FRANCE
Number of pages
25
Pages from-to
"A49/1"-"A49/25"
UT code for WoS article
000333798000049
EID of the result in the Scopus database
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