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| Open AccessThe imprint of star formation on stellar pulsations
The classical stellar evolution concept assumes that when the stars arrive on the main sequence, there is no traceable mark remains about their early evolutionary history. Here, the authors show that the accretion history leaves an imprint on the interior structure of the stars that are potentially detectable via asteroseismology.
- Thomas Steindl
- , Konstanze Zwintz
- & Eduard Vorobyov
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Article
| Open AccessGravitational-wave localization alone can probe origin of stellar-mass black hole mergers
Binary black hole mergers have recently been observed through the detection of gravitational wave signatures. The authors demonstrate that their association with active galactic nuclei can be made through a statistical spatial correlation.
- I. Bartos
- , Z. Haiman
- & S. Marka
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Article
| Open AccessFormation of the first three gravitational-wave observations through isolated binary evolution
Advanced LIGO has detected gravitational waves from two binary black hole mergers, plus a merger candidate. Here the authors use the COMPAS code to show that all three events can be explained by a single evolutionary channel via a common envelope phase, and characterize the progenitor metallicity and masses.
- Simon Stevenson
- , Alejandro Vigna-Gómez
- & Selma E. de Mink
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Article
| Open AccessEvidence from stable isotopes and 10Be for solar system formation triggered by a low-mass supernova
One hypothesis for solar system formation is gas compression by a nearby supernova, whose traces should be found in isotopic anomalies. Here the authors show that this mechanism is viable only if the triggering event was a low-mass supernova, looking at short-lived 10Be and lack of anomalies in stable isotopes.
- Projjwal Banerjee
- , Yong-Zhong Qian
- & W C Haxton