MIKULÁŠEK, Zdeněk, Augustin SKOPAL, Miloslav ZEJDA, Ondřej PEJCHA, Luboš KOHOUTEK, David MOTL, A. A. VITTONE and L. ERRICO. Light Variations of the Anomalous Central Star of Planetary Nebula Sh 2-71. In Active OB-Stars: Laboratories for Stellare and Circumstellar Physics, Proceedings of the conference held 29 August - 2 September, 2005 at Hokkai-Gakuen University, Sapporo, Japan. San Francisco: Astronomical Society of the Pacific, 2005, p. 469-471.
Other formats:   BibTeX LaTeX RIS
Basic information
Original name Light Variations of the Anomalous Central Star of Planetary Nebula Sh 2-71
Name in Czech Světelné změny anomální centrální hvězdy planetární mlhoviny Sh 2-71
Authors MIKULÁŠEK, Zdeněk (203 Czech Republic, guarantor), Augustin SKOPAL (703 Slovakia), Miloslav ZEJDA (203 Czech Republic), Ondřej PEJCHA (203 Czech Republic), Luboš KOHOUTEK (276 Germany), David MOTL (203 Czech Republic), A. A. VITTONE (380 Italy) and L. ERRICO (380 Italy).
Edition San Francisco, Active OB-Stars: Laboratories for Stellare and Circumstellar Physics, Proceedings of the conference held 29 August - 2 September, 2005 at Hokkai-Gakuen University, Sapporo, Japan, p. 469-471, 3 pp. 2005.
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
RIV identification code RIV/00216224:14310/05:00012965
Organization unit Faculty of Science
UT WoS 000246180400067
Keywords in English planetary nebulae; variable stars
Tags planetary nebulae, variable stars
Tags International impact, Reviewed
Changed by Changed by: doc. RNDr. Miloslav Zejda, Ph.D., učo 169695. Changed: 24/6/2009 11:52.
Abstract
We present an analysis of light variations in UBVRI of the anomalous object in the center of planetary nebula Sh 2-71. We refined the linear ephemeris of the light maxima to JDmax = 2449862.0 + 68.101 (E-96), but also identified long-term, obviously non-periodic variations. The latter manifest themselves in large O-C shifts, a variable profile of light curves (hereafter LC) and changes in the mean brightness of the object. Our spectroscopic observations suggested the presence of a superdense nebula in the center of Sh 2-71.
Abstract (in Czech)
Předkládáme rozbor světelných změn v UBVRI anomálního objektu v centru planetární mlhoviny Sh 2-71. Zpřesnili jsme lineární efemeridu maxima jasnosti na JDmax = 2449862.0 + 68.101 (E-96), současně jsme též identifikovali dlouhodobé, zřejmě aperiodické variace, jež se projevují velkými posuvy (O-C), změnami profilů světelných křivek a změnami střední jasnosti objektu. Naše spektroskopická pozorování ukazují na přítomnost suprahusté mlhoviny v centru Sh 2-71.
Links
GA205/04/1267, research and development projectName: Okolohvězdné obálky horkých hvězd
Investor: Czech Science Foundation, Circumstellar envelopes of hot stars
ME 128, research and development projectName: Alternativní přístupy k financování celoživotního učení
PrintDisplayed: 5/5/2024 02:49