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Scientific paper - Original scientific paper
Tracking massive pairs
Contributions of the Astronomical Observatory Skalnaté Pleso, 49 (2019), 2; 252-257. urn:nbn:hr:217:647221
Ratajczak, M.; Pigulski, A.; Pavlovski, K.

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Ratajczak, M., Pigulski, A. & Pavlovski, K. (2019). Tracking massive pairs. Contributions of the Astronomical Observatory Skalnaté Pleso, 49. (2), 252-257. Retrieved from https://urn.nsk.hr/urn:nbn:hr:217:647221

Ratajczak, M., et al. "Tracking massive pairs." Contributions of the Astronomical Observatory Skalnaté Pleso, vol. 49, no. 2, 2019, pp. 252-257. https://urn.nsk.hr/urn:nbn:hr:217:647221

Ratajczak, M., A. Pigulski and K. Pavlovski. "Tracking massive pairs." Contributions of the Astronomical Observatory Skalnaté Pleso 49, no. 2 (2019): 252-257. https://urn.nsk.hr/urn:nbn:hr:217:647221

Ratajczak, M., Pigulski, A. and Pavlovski, K. (2019) 'Tracking massive pairs', Contributions of the Astronomical Observatory Skalnaté Pleso, 49(2), pp. 252-257. Available at: https://urn.nsk.hr/urn:nbn:hr:217:647221 (Accessed 20 April 2024)

Ratajczak M, Pigulski A, Pavlovski K. Tracking massive pairs. Contributions of the Astronomical Observatory Skalnaté Pleso [Internet]. 2019 [cited 2024 April 20];49(2):252-257. Available at: https://urn.nsk.hr/urn:nbn:hr:217:647221

M. Ratajczak, A. Pigulski and K. Pavlovski, "Tracking massive pairs", Contributions of the Astronomical Observatory Skalnaté Pleso, vol. 49, no. 2, pp. 252-257, 2019. [Online]. Available at: https://urn.nsk.hr/urn:nbn:hr:217:647221. [Accessed: 20 April 2024]

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Metadata
Title (english)Tracking massive pairs
Title (english)Tracing massive pairs
AuthorM. Ratajczak
AuthorA. Pigulski
AuthorK. Pavlovski
Author's institutionUniversity of Zagreb
Faculty of Science
(Department of Physics)
Scientific / art field,
discipline and subdiscipline		NATURAL SCIENCES
Physics
Astronomy and Astrophysics
Abstract (english)
The analysis of eclipsing binaries with massive components enables to test stellar evolution models and track selected aspects of the structure of early-type stars. Stellar pairs with B-type components may serve to find tighter constraints on the mechanisms of convective core overshooting or masses ofβCephei-type stars. We present the results of an analysis of several eclipsing binaries – N Sco, LS CMa, andδVel – observed by BRITE-Constellation satellites and followed by a wide range of ground-based telescopes.
Keywords (english)
Languageenglish
Publication typeScientific paper - Original scientific paper
Publication statusPublished
Peer reviewPeer review - international
Publication versionPublished version
Journal titleContributions of the Astronomical Observatory Skalnaté Pleso
Numberingvol. 49, no. 2, pp. 252-257
p-ISSN1335-1842
URN:NBNurn:nbn:hr:217:647221
Publication2019
ProjectNumber: IP-2014-09-8656
Title (croatian): Zvijezde i prašina: struktura, sastav i interakcija
Acronym: STARDUST
Leader: Krešimir Pavlovski
Jurisdiction: Croatia
Funding stream: IP
Document URLhttps://www.ta3.sk/caosp/Eedition/Abstracts/2019/Vol_49/No_2/pp252-257_abstract.html
Type of resourceText
Access conditionsOpen access
Terms of useLicence Attribution 4.0 International (CC BY 4.0) icon
Public noteEach CAOSP article is published by the Astronomical Institute (owner of the copyright) as an Open Access article, under the terms of the Creative Commons Attribution License, which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited. Received: October 18, 2018. Accepted: January 22, 2019.
Created on2020-08-18 09:43:43