T
T. Kamiński
Researcher at Max Planck Society
Publications - 34
Citations - 1833
T. Kamiński is an academic researcher from Max Planck Society. The author has contributed to research in topics: Stars & Red supergiant. The author has an hindex of 20, co-authored 34 publications receiving 1596 citations. Previous affiliations of T. Kamiński include Harvard University & European Southern Observatory.
Papers
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Journal ArticleDOI
V1309 Scorpii: merger of a contact binary
R. Tylenda,Marcin Hajduk,T. Kamiński,Andrzej Udalski,Igor Soszyński,Michał K. Szymański,M. Kubiak,Grzegorz Pietrzyński,Grzegorz Pietrzyński,Radosław Poleski,Łukasz Wyrzykowski,Krzysztof Ulaczyk +11 more
TL;DR: In this paper, the authors investigated the nature of the observed short-term variability of the progenitor of V1309-Sco and found that the binary was a contact binary with an orbital period of 1.4 days.
Journal ArticleDOI
V1309 Scorpii: merger of a contact binary
R. Tylenda,Marcin Hajduk,T. Kamiński,Andrzej Udalski,Igor Soszyński,Michał K. Szymański,M. Kubiak,Grzegorz Pietrzyński,Grzegorz Pietrzyński,Radosław Poleski,Łukasz Wyrzykowski,Krzysztof Ulaczyk +11 more
TL;DR: In this paper, the authors investigate the nature of V1309 Sco and find that the progenitor was a contact binary with an orbital period of ~1.4 days.
Journal ArticleDOI
H2D+ observations give an age of at least one million years for a cloud core forming Sun-like stars
Sandra Brünken,Olli Sipilä,E. T. Chambers,Jorma Harju,Paola Caselli,Oskar Asvany,Cornelia E. Honingh,T. Kamiński,Karl M. Menten,Jürgen Stutzki,Stephan Schlemmer +10 more
TL;DR: Observations of ortho- and para-H2D+ emission and absorption from the dense cloud core hosting IRAS 16293-2422 A/B, a group of nascent solar-type stars, find that the dense core has been chemically processed for at least one million years.
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OGLE-2002-BLG-360: from a gravitational microlensing candidate to an overlooked red transient
R. Tylenda,T. Kamiński,Andrzej Udalski,Igor Soszyński,Radosław Poleski,Michał K. Szymański,M. Kubiak,Grzegorz Pietrzyński,S. Kozlowski,P. Pietrukowicz,Krzysztof Ulaczyk,L. Wyrzykowski +11 more
TL;DR: In this paper, the spectral energy distribution (SED) of OGLE-2002-BLG-360 was analyzed using a simple model of a star surrounded by a dusty envelope, which was used to interpret the observed SED.
Journal ArticleDOI
OGLE-2002-BLG-360: from a gravitational microlensing candidate to an overlooked red transient
R. Tylenda,T. Kamiński,Andrzej Udalski,Igor Soszyński,Radosław Poleski,Radosław Poleski,Michał K. Szymański,M. Kubiak,Grzegorz Pietrzyński,Grzegorz Pietrzyński,S. Kozlowski,P. Pietrukowicz,Krzysztof Ulaczyk,Łukasz Wyrzykowski +13 more
TL;DR: In this article, the spectral energy distribution (SED) of OGLE-2002-BLG-360 was analyzed using a simple model of a star surrounded by a dusty envelope, which was used to interpret the observed SED.