Zobrazeno 1 - 10
of 4 177
pro vyhledávání: '"Gossage"'
Autor:
Rocha, Kyle Akira, Hur, Rachel, Kalogera, Vicky, Gossage, Seth, Sun, Meng, Doctor, Zoheyr, Andrews, Jeff J., Bavera, Simone S., Briel, Max, Fragos, Tassos, Kovlakas, Konstantinos, Kruckow, Matthias U., Misra, Devina, Xing, Zepei, Zapartas, Emmanouil
We investigate Roche lobe overflow mass transfer (MT) in eccentric binary systems between stars and compact objects (COs), modeling the coupled evolution of both the star and the orbit due to eccentric MT (eMT) in a self-consistent framework. We impl
Externí odkaz:
http://arxiv.org/abs/2411.11840
Autor:
Srivastava, Philipp M., Demir, Ugur, Katsaggelos, Aggelos, Kalogera, Vicky, Teng, Elizabeth, Fragos, Tassos, Andrews, Jeff J., Bavera, Simone S., Briel, Max, Gossage, Seth, Kovlakas, Konstantinos, Kruckow, Matthias U., Liotine, Camille, Rocha, Kyle A., Sun, Meng, Xing, Zepei, Zapartas, Emmanouil
Modeling of large populations of binary stellar systems is an intergral part of a many areas of astrophysics, from radio pulsars and supernovae to X-ray binaries, gamma-ray bursts, and gravitational-wave mergers. Binary population synthesis codes tha
Externí odkaz:
http://arxiv.org/abs/2411.02586
Autor:
Andrews, Jeff J., Bavera, Simone S., Briel, Max, Chattaraj, Abhishek, Dotter, Aaron, Fragos, Tassos, Gallegos-Garcia, Monica, Gossage, Seth, Kalogera, Vicky, Kasdagli, Eirini, Katsaggelos, Aggelos, Kimball, Chase, Kovlakas, Konstantinos, Kruckow, Matthias U., Liotine, Camille, Misra, Devina, Rocha, Kyle A., Souropanis, Dimitris, Srivastava, Philipp M., Sun, Meng, Teng, Elizabeth, Xing, Zepei, Zapartas, Emmanouil, Zevin, Michael
Whether considering rare astrophysical events on cosmological scales or unresolved stellar populations, accurate models must account for the integrated contribution from the entire history of star formation upon which that population is built. Here,
Externí odkaz:
http://arxiv.org/abs/2411.02376
Autor:
Xing, Zepei, Kalogera, Vicky, Fragos, Tassos, Andrews, Jeff J., Bavera, Simone S., Briel, Max, Gossage, Seth, Kovlakas, Konstantinos, Kruckow, Matthias U., Rocha, Kyle A., Sun, Meng, Srivastava, Philipp M., Zapartas, Emmanouil
The existence of a mass gap of $3-5\,M_{\odot}$ between the heaviest neutron stars (NSs) and the lightest black holes (BHs), inferred from the BH mass distribution in low mass X-ray binaries (LMXBs), has been suggested for decades. The recently repor
Externí odkaz:
http://arxiv.org/abs/2410.20415
Autor:
Gossage, Seth, Kiman, Rocio, Monsch, Kristina, Medina, Amber A., Drake, Jeremy J., Garraffo, Cecilia, Yuxi, Lu, Wing, Joshua D., Wright, Nicholas J.
The relationship between magnetic activity and Rossby number is one way through which stellar dynamos can be understood. Using measured rotation rates and X-ray to bolometric luminosity ratios of an ensemble of stars, we derive empirical convective t
Externí odkaz:
http://arxiv.org/abs/2410.20000
Autor:
Kruckow, Matthias U., Andrews, Jeff J., Fragos, Tassos, Holl, Berry, Bavera, Simone S., Briel, Max, Gossage, Seth, Kovlakas, Konstantinos, Rocha, Kyle A., Sun, Meng, Srivastava, Philipp M., Xing, Zepei, Zapartas, Emmanouil
Context. The black holes discovered using Gaia, especially Gaia BH1 and BH2, have low mass companions of solar-like metallicity in wide orbits. For standard isolated binary evolution formation channels including interactions such an extreme mass rati
Externí odkaz:
http://arxiv.org/abs/2410.18501
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
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
