Conference item

Massive binary mergers and thorne-zytkow objects

Abstract:: Some 10% of all massive stars are predicted to merge completely with a companion star. Here we review the different types of mergers and how they may produce unusual objects such as the anomalous progenitor of SN 1987A, gamma-ray burst sources and Thorne-Zytkow objects.

Publication status:: Published

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APA Style

Podsiadlowski, P. (2007). Massive binary mergers and thorne-zytkow objects. Workshop on Massive Stars in Interacting Binaries, 367, 541–548.

MLA Style

Podsiadlowski, P. “Massive Binary Mergers and Thorne-Zytkow Objects.” Workshop on Massive Stars in Interacting Binaries, vol. 367, 2007, pp. 541–48.

Chicago Style

Podsiadlowski, P. 2007. “Massive Binary Mergers and Thorne-Zytkow Objects.” In Workshop on Massive Stars in Interacting Binaries, 367:541–48.
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Authors

+ Podsiadlowski, P More by this author

Institution:: University of Oxford
Division:: MPLS
Department:: Physics
Sub department:: Astrophysics
Role:: Author

Journal:: MASSIVE STARS IN INTERACTING BINARIES More from this journal
Volume:: 367
Pages:: 541-548
Publication date:: 2007-01-01
Event title:: Workshop on Massive Stars in Interacting Binaries
ISBN:: 9781583812358

Keywords:: ENVELOPE

DEGENERATE NEUTRON CORES

TRIPLE RING NEBULA

PROGENITORS

SN 1987A

STARS

EVOLUTION

INFALL

HYPERNOVAE

GAMMA-RAY BURSTS
Pubs id:: pubs:11835
UUID:: uuid:7e9a30fc-a375-4efd-819d-e04ea9b45a3e
Local pid:: pubs:11835
Source identifiers:: 11835
Deposit date:: 2012-12-19
ARK identifier:: ark:/29072/ora_7e9a30fca3754efd819de04ea9b45a3e

Terms of use

Copyright date:: 2007

Licence:: Terms and Conditions of Use for Oxford University Research Archive

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