ZEJDA, Miloslav, Ernst PAUNZEN and Zdeněk MIKULÁŠEK. Delta a Photometric survey of the small magellanic cloud. In Elizabeth R. Griffin. Symposium S339 (Southern Horizons in Time-Domain Astronomy). Neuveden: Cambridge University Press, 2019, p. 349-352. ISSN 1743-9213. Available from: https://dx.doi.org/10.1017/S1743921318002995.
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Basic information
Original name Delta a Photometric survey of the small magellanic cloud
Authors ZEJDA, Miloslav (203 Czech Republic, guarantor, belonging to the institution), Ernst PAUNZEN (40 Austria, belonging to the institution) and Zdeněk MIKULÁŠEK (203 Czech Republic, belonging to the institution).
Edition Neuveden, Symposium S339 (Southern Horizons in Time-Domain Astronomy), p. 349-352, 4 pp. 2019.
Publisher Cambridge University Press
Other information
Original language English
Type of outcome Proceedings paper
Field of Study 10308 Astronomy
Country of publisher United Kingdom of Great Britain and Northern Ireland
Confidentiality degree is not subject to a state or trade secret
Publication form printed version "print"
WWW URL
RIV identification code RIV/00216224:14310/19:00108285
Organization unit Faculty of Science
ISSN 1743-9213
Doi http://dx.doi.org/10.1017/S1743921318002995
Keywords in English Stars: chemically peculiar; stars: emission-line; Be; galaxies: Small Magellanic Cloud; techniques: photometric: Detla a
Tags rivok
Tags International impact, Reviewed
Changed by Changed by: Mgr. Marie Šípková, DiS., učo 437722. Changed: 21/4/2020 17:56.
Abstract
The narrow-band delta a photometric system measures the flux depression at lambda 5200 angstrom by comparing the flux at the band centre to adjacent regions. It has been shown that virtually all peculiar stars with magnetic fields (mCPs) have significant positive delta a values (of up to +100 mmag), whereas Be/Ae/B[e] and metal weak stars (including lambda Bootis types) exhibit significant negative values of delta a. By using this photometric system we are therefore able to detect chemically peculiar (CP), emission types and metal-weak stars in an efficient way. The poster presented the first results of our survey of the Small Magellanic Cloud. In the selected field we found only 0.5 % of bona fide CP stars against 15 % in our Galaxy.
Links
GA16-01116S, research and development projectName: Atmosféry a okolohvězdné prostředí magnetických horkých hvězd
Investor: Czech Science Foundation
LG15010, research and development projectName: F. Magellanes: projekt podpory studia hvězd a hvězdných soustav na základě pozorování ze Země a z kosmického prostoru (Acronym: Magellan2015)
Investor: Ministry of Education, Youth and Sports of the CR
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