Search Results - "Srivastava, Philipp M."

POSYDON: A General-purpose Population Synthesis Code with Detailed Binary-evolution Simulations by Fragos, Tassos, J. Andrews, Jeff, Bavera, Simone S., Berry, Christopher P. L., Coughlin, Scott, Dotter, Aaron, Giri, Prabin, Kalogera, Vicky, Katsaggelos, Aggelos, Kovlakas, Konstantinos, Lalvani, Shamal, Misra, Devina, Srivastava, Philipp M., Qin, Ying, Rocha, Kyle A., Román-Garza, Jaime, Serra, Juan Gabriel, Stahle, Petter, Sun, Meng, Teng, Xu, Trajcevski, Goce, Tran, Nam Hai, Xing, Zepei, Zapartas, Emmanouil, Zevin, Michael

“…Abstract Most massive stars are members of a binary or a higher-order stellar system, where the presence of a binary companion can decisively alter their…”
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To Be or Not To Be: The Role of Rotation in Modeling Galactic Be X-Ray Binaries by 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

“…Abstract 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…”
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Investigating the Lower Mass Gap with Low-mass X-Ray Binary Population Synthesis by Siegel, Jared C., Kiato, Ilia, Kalogera, Vicky, Berry, Christopher P. L., Maccarone, Thomas J., Breivik, Katelyn, Andrews, Jeff J., Bavera, Simone S., Dotter, Aaron, Fragos, Tassos, Kovlakas, Konstantinos, Misra, Devina, Rocha, Kyle A., Srivastava, Philipp M., Sun, Meng, Xing, Zepei, Zapartas, Emmanouil

“…Abstract Mass measurements from low-mass black hole X-ray binaries (LMXBs) and radio pulsars have been used to identify a gap between the most massive neutron…”
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A Black Hole Kicked at Birth: MAXI J1305-704 by Kimball, Chase, Imperato, Sam, Kalogera, Vicky, Rocha, Kyle A., Doctor, Zoheyr, Andrews, Jeff J., Dotter, Aaron, Zapartas, Emmanouil, Bavera, Simone S., Kovlakas, Konstantinos, Fragos, Tassos, Srivastava, Philipp M., Misra, Devina, Sun, Meng, Xing, Zepei

“…Abstract When a compact object is formed in a binary, any mass lost during core collapse will impart a kick on the binary’s center of mass. Asymmetries in this…”
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The formation of merging black holes with masses beyond 30 M⊙ at solar metallicity by Bavera, Simone S., Fragos, Tassos, Zapartas, Emmanouil, Andrews, Jeff J., Kalogera, Vicky, Berry, Christopher P. L., Kruckow, Matthias, Dotter, Aaron, Kovlakas, Konstantinos, Misra, Devina, Rocha, Kyle A., Srivastava, Philipp M., Sun, Meng, Xing, Zepei

“…Gravitational-wave astronomy has revealed a population of stellar-mass black holes more massive than observed previously by other means. The maximum mass of…”
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Irregularly Sampled Time Series Interpolation for Detailed Binary Evolution Simulations by 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…”
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Mass-gap Black Holes in Coalescing Neutron Star Black Hole Binaries by 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…”
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The Formation of Black Holes in Non-interacting, Isolated Binaries. Gaia Black Holes as Calibrators of Stellar Winds From Massive Stars by 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…”
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Emulators for stellar profiles in binary population modeling by 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…”
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To Be or not to Be: the role of rotation in modeling Galactic Be X-ray Binaries by 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…”
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Formation of Wind-Fed Black Hole High-mass X-ray Binaries: The Role of Roche-lobe-Overflow Post Black-Hole Formation by 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)…”
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Exploring the nature of ultra-luminous X-ray sources across stellar population ages using detailed binary evolution calculations by Misra, Devina, Kovlakas, Konstantinos, Fragos, Tassos, Andrews, Jeff J, Bavera, Simone S, Zapartas, Emmanouil, Xing, Zepei, Dotter, Aaron, Rocha, Kyle Akira, Srivastava, Philipp M, Sun, Meng

“…A&A 682, A69 (2024) Ultra-luminous X-ray sources (ULXs) are sources observed to exceed the Eddington limit of a stellar-mass black hole (BH). A fraction of ULX…”
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POSYDON Version 2: Population Synthesis with Detailed Binary-Evolution Simulations across a Cosmological Range of Metallicities by 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…”
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From ZAMS to Merger: Detailed Binary Evolution Models of Coalescing Neutron Star-Black Hole Systems at Solar Metallicity by Xing, Zepei, Bavera, Simone S, Fragos, Tassos, Kruckow, Matthias U, Román-Garza, Jaim, Andrews, Jeff J, Dotter, Aaron, Kovlakas, Konstantinos, Misra, Devina, Srivastava, Philipp M, Rocha, Kyle A, Sun, Meng, Zapartas, Emmanouil

“…Neutron star $-$ black hole (NSBH) merger events bring us new opportunities to constrain theories of stellar and binary evolution, and understand the nature of…”
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X-ray luminosity function of high-mass X-ray binaries: Studying the signatures of different physical processes using detailed binary evolution calculations by Misra, Devina, Kovlakas, Konstantinos, Fragos, Tassos, Lazzarini, Margaret, Bavera, Simone S, Lehmer, Bret D, Zezas, Andreas, Zapartas, Emmanouil, Xing, Zepei, Andrews, Jeff J, Dotter, Aaron, Rocha, Kyle A, Srivastava, Philipp M, Sun, Meng

“…A&A 672, A99 (2023) The ever-expanding observational sample of X-ray binaries (XRBs) makes them excellent laboratories for constraining binary evolution…”
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The formation of $30\,M_\odot$ merging black holes at solar metallicity by Bavera, Simone S, Fragos, Tassos, Zapartas, Emmanouil, Andrews, Jeff J, Kalogera, Vicky, Berry, Christopher P. L, Kruckow, Matthias, Dotter, Aaron, Kovlakas, Konstantinos, Misra, Devina, Rocha, Kyle A, Srivastava, Philipp M, Sun, Meng, Xing, Zepei

“…The maximum mass of black holes formed in isolated binaries is determined by stellar winds and the interactions between the binary components. We consider for…”
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Investigating the Lower Mass Gap with Low Mass X-ray Binary Population Synthesis by Siegel, Jared C, Kiato, Ilia, Kalogera, Vicky, Berry, Christopher P. L, Maccarone, Thomas J, Breivik, Katelyn, Andrews, Jeff J, Bavera, Simone S, Dotter, Aaron, Fragos, Tassos, Kovlakas, Konstantinos, Misra, Devina, Rocha, Kyle A, Srivastava, Philipp M, Sun, Meng, Xing, Zepei, Zapartas, Emmanouil

“…Mass measurements from low-mass black hole X-ray binaries (LMXBs) and radio pulsars have been used to identify a gap between the most massive neutron stars…”
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POSYDON: A General-Purpose Population Synthesis Code with Detailed Binary-Evolution Simulations by Fragos, Tassos, Andrews, Jeff J, Bavera, Simone S, Berry, Christopher P. L, Coughlin, Scott, Dotter, Aaron, Giri, Prabin, Kalogera, Vicky, Katsaggelos, Aggelos, Kovlakas, Konstantinos, Lalvani, Shamal, Misra, Devina, Srivastava, Philipp M, Qin, Ying, Rocha, Kyle A, Roman-Garza, Jaime, Serra, Juan Gabriel, Stahle, Petter, Sun, Meng, Teng, Xu, Trajcevski, Goce, Tran, Nam Hai, Xing, Zepei, Zapartas, Emmanouil, Zevin, Michael

“…Most massive stars are members of a binary or a higher-order stellar systems, where the presence of a binary companion can decisively alter their evolution via…”
Get full text