Zobrazeno 1 - 10
of 4 144
pro vyhledávání: '"Gossage"'
Autor:
Teng, Elizabeth, Demir, Ugur, Doctor, Zoheyr, Srivastava, Philipp M., Lalvani, Shamal, Kalogera, Vicky, Katsaggelos, Aggelos, Andrews, Jeff J., Bavera, Simone S., Briel, Max M., Gossage, Seth, Kovlakas, Konstantinos, Kruckow, Matthias U., Rocha, Kyle Akira, Sun, Meng, Xing, Zepei, Zapartas, Emmanouil
Knowledge about the internal physical structure of stars is crucial to understanding their evolution. The novel binary population synthesis code POSYDON includes a module for interpolating the stellar and binary properties of any system at the end of
Externí odkaz:
http://arxiv.org/abs/2410.11105
Autor:
Zapartas, E., de Wit, S., Antoniadis, K., Muñoz-Sanchez, G., Souropanis, D., Bonanos, A. Z., Maravelias, G., Kovlakas, K., Kruckow, M. U., Fragos, T., Andrews, J. J., Bavera, S. S., Briel, M., Gossage, S., Kasdagli, E., Rocha, K. A., Sun, M., Srivastava, P. M., Xing, Z.
The rate and mechanism of mass loss of red supergiants (RSGs) remain poorly understood, especially at low metallicities. Motivated by the new empirical prescription by Yang et al. 2023, based on the largest and most complete sample in the Small Magel
Externí odkaz:
http://arxiv.org/abs/2410.07335
Autor:
Xing, Zepei, Fragos, Tassos, Zapartas, Emmanouil, Kwan, Tom M., Dai, Lixin, Mandel, Ilya, Kruckow, Matthias U., Briel, Max, Andrews, Jeff J., Bavera, Simone S., Gossage, Seth, Kovlakas, Konstantinos, Rocha, Kyle A., Sun, Meng, Srivastava, Philipp M.
The three dynamically confirmed wind-fed black hole high-mass X-ray binaries (BH-HMXBs) are suggested to all contain a highly spinning black hole (BH). However, based on the theories of efficient angular momentum transport inside the stars, we expect
Externí odkaz:
http://arxiv.org/abs/2407.00200
Motivated by measurements of the rotation speed of accretor stars in post-mass-transfer (post-MT) systems, we investigate how magnetic braking affects the spin-down of individual stars during binary evolution with the MESAbinary module. Unlike the co
Externí odkaz:
http://arxiv.org/abs/2403.17279
Autor:
Rocha, Kyle Akira, Kalogera, Vicky, Doctor, Zoheyr, Andrews, Jeff J., Sun, Meng, Gossage, Seth, Bavera, Simone S., Fragos, Tassos, Kovlakas, Konstantinos, Kruckow, Matthias U., Misra, Devina, Srivastava, Philipp M., Xing, Zepei, Zapartas, Emmanouil
Be X-ray binaries (Be-XRBs) are one of the largest subclasses of high-mass X-ray binaries, comprised of a rapidly rotating Be star and neutron star companion in an eccentric orbit, intermittently accreting material from a decretion disk around the do
Externí odkaz:
http://arxiv.org/abs/2403.07172
Galactic archaeology largely relies on precise ages of distant evolved stars in the Milky Way. Nowadays, asteroseismology can deliver ages for many red giants observed with high-cadence, high-precision photometric space missions. Our aim is to quanti
Externí odkaz:
http://arxiv.org/abs/2402.05168
Experiences of Serving and Ex-Serving Members With the PTSD Coach Australia App: Mixed Methods Study
Autor:
Shakespeare-Finch, Jane, Alichniewicz, Karolina K, Strodl, Esben, Brown, Kelly, Quinn, Catherine, Hides, Leanne, White, Angela, Gossage, Gabrial, Poerio, Loretta, Batras, Dimitri, Jackson, Samantha, Styles, Jess, Kavanagh, David
Publikováno v:
Journal of Medical Internet Research, Vol 22, Iss 10, p e18447 (2020)
BackgroundPTSD Coach Australia is an app for serving and ex-serving defense members and was adapted for the Australian context in 2013 from PTSD Coach, which was created in the United States. ObjectiveThis study aimed to provide a user-centered eval
Externí odkaz:
https://doaj.org/article/d17202179ddc417cb4622d90e0bad4e1
Autor:
Li, Gang, Aerts, Conny, Bedding, Timothy R., Fritzewski, Dario J., Murphy, Simon J., Van Reeth, Timothy, Montet, Benjamin T., Jian, Mingjie, Mombarg, Joey S. G., Gossage, Seth, Sreenivas, K. R.
Publikováno v:
A&A 686, A142 (2024)
Asteroseismic modelling of isolated star presents significant challenges due to the difficulty in accurately determining stellar parameters, particularly the stellar age. These challenges can be overcomed by observing stars in open clusters, whose co
Externí odkaz:
http://arxiv.org/abs/2311.16991
Wind Roche-lobe Overflow in Low-Mass Binaries: Exploring the Origin of Rapidly Rotating Blue Lurkers
Autor:
Sun, Meng, Levina, Sasha, Gossage, Seth, Kalogera, Vicky, Leiner, Emily M., Geller, Aaron M., Doctor, Zoheyr
Wind Roche-Lobe Overflow (WRLOF) is a mass-transfer mechanism proposed by Mohamed and Podsiadlowski (2007) for stellar binaries wherein the wind acceleration zone of the donor star exceeds its Roche lobe radius, allowing stellar wind material to be t
Externí odkaz:
http://arxiv.org/abs/2311.07528