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Books > Science & Mathematics > Physics > Applied physics & special topics > Astrophysics
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Observational Imprints of Binary Evolution on B- and Be-star Populations (Hardcover, 1st ed. 2022)
Loot Price: R3,321
Discovery Miles 33 210
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Observational Imprints of Binary Evolution on B- and Be-star Populations (Hardcover, 1st ed. 2022)
Series: Springer Theses
Expected to ship within 18 - 22 working days
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This book presents novel observational evidence toward detecting
and characterizing the products of massive, interacting binary
stars. As a majority of massive stars are born in close binary
systems, a large number of so-called massive binary interaction
products are predicted to exist; however, few have been identified
so far. Based on observations with the largest telescopes around
the world, equipped with state-of-the-art instrumentation, this
book helps to remedy this situation. In her outstanding PhD-thesis
Julia Bodensteiner identifies a new class of post-interaction
binaries in a short-lived phase just briefly after the initially
more massive star has been stripped of part of its envelope. She
further provides new evidence for the Be phenomenon to largely
result from binary interactions. These results represented a new
and testable prediction for the evolution of these stars and opened
up a new way forward for identifying hundreds of post-interaction
products. Finally, using the MUSE integral field spectrograph at
the Very Large Telescope in Chile, the author presents a novel
spectroscopic campaign focusing on the 40 Myr-old star cluster NGC
330 in the Small Magellanic Clouds. Combined with photometric
observations from the Hubble Space Telescope, the MUSE data allow
to characterize the entire massive star population of NGC 330,
revealing their multiplicity properties and rotational velocities
and providing unique observational constraints on their (binary)
evolution history. This is made possible by the developments of
novel numerical methods allowing to extract star spectra from the
MUSE integral field spectroscopic data and to characterize their
properties by the simultaneous comparison of MUSE spectroscopy and
Hubble photometry with atmospheric models. This book is a partly
re-written version of the author's thesis offering a highly
readable coherent text presenting not only new insights into the
properties of binary interaction products but also giving students
an excellent introduction into the field.
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