Zobrazeno 1 - 10
of 27
pro vyhledávání: '"Luke Chamandy"'
Publikováno v:
The Astrophysical Journal, Vol 966, Iss 1, p 78 (2024)
Galactic dynamo models have generally relied on input parameters that are very challenging to constrain. We address this problem by developing a model that uses observable quantities as input: the galaxy rotation curve, the surface densities of the g
Externí odkaz:
https://doaj.org/article/fa5d9c4378c249e597dcc7c1d80838d9
Autor:
Luke Chamandy, Anvar Shukurov
Publikováno v:
Galaxies, Vol 8, Iss 3, p 56 (2020)
Galactic dynamo models take as input certain parameters of the interstellar turbulence, most essentially the correlation time τ, root-mean-square turbulent speed u, and correlation scale l. However, these quantities are difficult, or, in the case of
Externí odkaz:
https://doaj.org/article/474365fe5efd46c5b12b954829da6773
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 514:3041-3057
It has long been speculated that jet feedback from accretion onto the companion during a common envelope (CE) event could affect the orbital evolution and envelope unbinding process, but this conjecture has heretofore remained largely untested. We pr
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::74ddc96169bd1ebb39962976b451ce9b
https://doi.org/10.1093/mnras/stac1529
https://doi.org/10.1093/mnras/stac1529
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 494:5333-5349
During the common envelope binary interaction, the expanding layers of the gaseous common envelope recombine and the resulting recombination energy has been suggested as a contributing factor to the ejection of the envelope. In this paper we perform
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::c63551ddce15cbef66989733ca87b693
https://doi.org/10.1093/mnras/staa937
https://doi.org/10.1093/mnras/staa937
Autor:
Jonathan Carroll-Nellenback, Yangyuxin Zou, Eric G. Blackman, Luke Chamandy, Adam Frank, Yisheng Tu
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 490:3727-3739
We compute the forces, torque and rate of work on the companion-core binary due to drag in global simulations of common envelope (CE) evolution for three different companion masses. Our simulations help to delineate regimes when conventional analytic
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::bb8c58d46d1c412409eb1b48ce5eeeb0
https://doi.org/10.1093/mnras/stz2813
https://doi.org/10.1093/mnras/stz2813
Common envelope (CE) evolution is a critical but still poorly understood progenitor phase of many high-energy astrophysical phenomena. Although 3D global hydrodynamic CE simulations have become more common in recent years, those involving an asymptot
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::8b695f06cbc51f13cb6fba92e5235598
http://arxiv.org/abs/2004.06829
http://arxiv.org/abs/2004.06829
Many stars harbour multi-planet systems. As these stars expand late in their evolutions, the innermost planet may be engulfed, leading to a common envelope (CE) event. Even if this is insufficient to eject the envelope, it may expand the star further
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::956cd5fd245ea0cf606954266388add9
Autor:
Anvar Shukurov, Luke Chamandy
Publikováno v:
Galaxies, Vol 8, Iss 56, p 56 (2020)
Galaxies
Volume 8
Issue 3
Galaxies
Volume 8
Issue 3
Galactic dynamo models take as input certain parameters of the interstellar turbulence, most essentially the correlation time &tau
root-mean-square turbulent speed u, and correlation scale l. However, these quantities are difficult, or, in the c
root-mean-square turbulent speed u, and correlation scale l. However, these quantities are difficult, or, in the c
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::70f414b2924a0f3888e384aedc6d97d4
Autor:
Eric G. Blackman, Baowei Liu, Zhuo Chen, Bo Peng, Adam Frank, Jonathan Carroll-Nellenback, Yisheng Tu, Luke Chamandy, Jason Nordhaus
Publikováno v:
Proceedings of the International Astronomical Union. 14:235-238
Common envelope evolution (CEE) is presently a poorly understood, yet critical, process in binary stellar evolution. Characterizing the full 3D dynamics of CEE is difficult in part because simulating CEE is so computationally demanding. Numerical stu
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::09a62fdb883a051148b542f7a83d592d
https://doi.org/10.1017/s174392131800666x
https://doi.org/10.1017/s174392131800666x
Autor:
G Guidarelli, Zhuo Chen, Jonathan Carroll-Nellenback, Jason Nordhaus, Baowei Liu, Eric G. Blackman, Adam Frank, Luke Chamandy
Volume complete sky surveys provide evidence for a binary origin for the formation of isolated white dwarfs with magnetic fields in excess of a MegaGauss. Interestingly, not a single high-field magnetic white dwarf has been found in a detached system
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::54f3e23896d28ad02b3f31fefeb97080