PAUNZEN, Ernst, Jan JANÍK, Petr KURFÜRST, Jiří LIŠKA, Martin NETOPIL, Marek SKARKA and Miloslav ZEJDA. Tracing the B[e] Phenomenon with the Narrow-Band delta a Photometric System. In A. Miroshnichenko, S. Zharikov, D. Korcakova. The B[e] Phenomenom: Forty Years of Studies. 508th ed. San Francisco, USA: Astronomical Society of the Pacific, 2017, p. 143-148. ISBN 978-1-58381-900-5.
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Basic information
Original name Tracing the B[e] Phenomenon with the Narrow-Band delta a Photometric System
Name in Czech Tracing the B[e] Phenomenon with the Narrow-Band 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 (40 Austria, belonging to the institution), Marek SKARKA (203 Czech Republic) and Miloslav ZEJDA (203 Czech Republic, belonging to the institution).
Edition 508. vyd. San Francisco, USA, The B[e] Phenomenom: Forty Years of Studies, p. 143-148, 6 pp. 2017.
Publisher Astronomical Society of the Pacific
Other information
Original language English
Type of outcome Proceedings paper
Field of Study 10308 Astronomy
Country of publisher United States of America
Confidentiality degree is not subject to a state or trade secret
Publication form printed version "print"
RIV identification code RIV/00216224:14310/17:00096532
Organization unit Faculty of Science
ISBN 978-1-58381-900-5
UT WoS 000401591600021
Keywords (in Czech) photometry; delta a photometry; B[e] stars; Magellanic Clouds
Keywords in English photometry; delta a photometry; B[e] stars; Magellanic Clouds
Tags NZ, rivok
Tags International impact
Changed by Changed by: Ing. Nicole Zrilić, učo 240776. Changed: 24/3/2018 17:22.
Abstract
We present a case study and first results of the 3 filter narrow-band delta a photometric system to detect B[e] stars in an efficient way. One filter measures the flux at 5200 A where several Fe II emission lines are located. On the basis of available spectra, we investigated the expected area in the diagnostic tool of the delta a system, the so-called normality line, where these objects are located. They are well separated from all other known non-standard stars in the corresponding Teff (color) region. The first results of our photometric survey in the Magellanic Clouds are very promising and show the high potential of delta a photometry to significantly contribute to this research field.
Links
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
PrintDisplayed: 10/5/2024 00:08