Zobrazeno 1 - 6
of 6
pro vyhledávání: '"J. D. M. Dewi"'
Publikováno v:
Monthly Notices of the Royal Astronomical Society, 370, L6-L9. Oxford University Press
The starburst galaxy M82 at a distance of 12 million light years, is the host of an unusually bright $2.4-16\times 10^{40}$ erg/s X-ray point source, which is best explained by an accreting black hole $10^{2}$ to $10^4$ times more massive than the Su
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::e6f21da2343ade2139a4625a6ef7a115
https://dare.uva.nl/personal/pure/en/publications/the-ultraluminous-xray-source-in-m82-an-intermediatemass-black-hole-with-a-giant-companion(bee89b37-5b64-4eb4-b41e-3a765dca0ef4).html
https://dare.uva.nl/personal/pure/en/publications/the-ultraluminous-xray-source-in-m82-an-intermediatemass-black-hole-with-a-giant-companion(bee89b37-5b64-4eb4-b41e-3a765dca0ef4).html
Publikováno v:
Monthly Notices of the Royal Astronomical Society: Letters. 363:L71-L75
Double neutron stars (DNSs), binary systems consisting of a radio pulsar and a generally undetected second neutron star (NS), have proven to be excellent laboratories for testing the theory of general relativity. The seven systems discovered in our G
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::2e3238f97d4e63861948a3ecf89c89fc
https://doi.org/10.1111/j.1745-3933.2005.00085.x
https://doi.org/10.1111/j.1745-3933.2005.00085.x
Autor:
J. D. M. Dewi, William G. Newton, Ph. Podsiadlowski, Pierre Lesaffre, John C. Miller, Jirina Stone
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 361:1243-1249
The double pulsar J0737--3039 has become an important astrophysical laboratory for testing fundamental physics. Here we demonstrate that the low measured mass of Pulsar B can be used to constrain the equation of state of neutron star matter {\em unde
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::88eb34e5f4b48f3599f462261c031b91
https://doi.org/10.1111/j.1365-2966.2005.09253.x
https://doi.org/10.1111/j.1365-2966.2005.09253.x
Publikováno v:
Astrophysics and Space Science ISBN: 9781402040849
The evolution of young (≲10 Myr) star clusters with a density exceeding about 105 star pc−3 are strongly affected by physical stellar collisions during their early lifetime. In such environments the same star may participate in several tens to hu
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::93c1c6643d354dea9838c0677033cdd2
https://doi.org/10.1007/1-4020-4085-7_28
https://doi.org/10.1007/1-4020-4085-7_28
Publikováno v:
AIP Conference Proceedings.
The seven Galactic double neutron stars (DNS)s exhibit a relation between the pulsar spin period and the orbital eccentricity. We show that this relation can only be produced if the second neutron star received a kick that is substantially smaller (w
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::72de2105e3dcedbfb74e91d48d9515cb
https://doi.org/10.1063/1.2774924
https://doi.org/10.1063/1.2774924
We present the results of a systematic exploration of an alternative evolutionary scenario to form double neutron-star binaries, first proposed by Brown (1995), which does not involve a neutron star passing through a common envelope. In this scenario
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::8fe7da2cb86644cc52f59429bfc78e8b
http://arxiv.org/abs/astro-ph/0602510
http://arxiv.org/abs/astro-ph/0602510