Detailed Information on Publication Record
2019
AGB stars of the Magellanic Clouds as seen within the delta-a photometric system
PAUNZEN, Ernst, Jan JANÍK, Petr KURFÜRST, Jiří LIŠKA, Martin NETOPIL et. al.Basic information
Original name
AGB stars of the Magellanic Clouds as seen within the delta-a photometric system
Authors
PAUNZEN, Ernst (40 Austria, guarantor, belonging to the institution), Jan JANÍK (203 Czech Republic, belonging to the institution), Petr KURFÜRST (203 Czech Republic, belonging to the institution), Jiří LIŠKA (203 Czech Republic, belonging to the institution), Martin NETOPIL, Marek SKARKA (203 Czech Republic, belonging to the institution) and Miloslav ZEJDA (203 Czech Republic, belonging to the institution)
Edition
UK, Symposium S343 (Why Galaxies Care About AGB Stars: A Continuing Challenge through Cosmic Time), p. 487-488, 2 pp. 2019
Publisher
Cambridge University Press
Other information
Language
English
Type of outcome
Stať ve sborníku
Field of Study
10308 Astronomy
Country of publisher
United Kingdom of Great Britain and Northern Ireland
Confidentiality degree
není předmětem státního či obchodního tajemství
Publication form
electronic version available online
References:
RIV identification code
RIV/00216224:14310/19:00115532
Organization unit
Faculty of Science
ISSN
Keywords in English
Magellanic Clouds; stars: AGB and post-AGB; techniques: photometric
Tags
Tags
International impact, Reviewed
Změněno: 12/5/2021 15:38, Mgr. Marie Šípková, DiS.
Abstract
V originále
The a-index samples the flux of the 5200 angstrom region by comparing the flux at the center with the adjacent regions. The final intrinsic peculiarity index delta-a was defined as the difference between the individual a-values and the a-values of normal stars of the same colour (spectral type). Here we present, for the first time, a case study to detect and analyse Asymptotic Giant Branch (AGB) stars in the Magellanic Clouds. For this, we use our photometric survey of the Magellanic Clouds within the a-index. We find that AGB stars can be easily detected on the basis of their delta-a index in an efficient way.
Links
EF16_027/0008360, research and development project |
| ||
LH14300, research and development project |
|