Zobrazeno 1 - 10
of 113
pro vyhledávání: '"Paxton, B"'
Autor:
Farmer, R., Fields, C. E., Petermann, I., Dessart, Luc, Cantiello, M., Paxton, B., Timmes, F. X.
We explore the variation in single star 15-30 $\rm{M}_{\odot}$, non-rotating, solar metallicity, pre-supernova MESA models due to changes in the number of isotopes in a fully-coupled nuclear reaction network and adjustments in the mass resolution. Wi
Externí odkaz:
http://arxiv.org/abs/1611.01207
Autor:
Battino, U., Pignatari, M., Ritter, C., Herwig, F., Denisenkov, P., Hartogh, J. W. Den, Trappitsch, R., Hirschi, R., Freytag, B., Thielemann, F., Paxton, B.
The $s$-process nucleosynthesis in Asymptotic Giant Branch (AGB) stars depends on the modeling of convective boundaries. We present models and s-process simulations that adopt a treatment of convective boundaries based on the results of hydrodynamic
Externí odkaz:
http://arxiv.org/abs/1605.06159
We investigate the evolution of super-AGB thermal pulse (TP) stars for a range of metallicities (Z) and explore the effect of convective boundary mixing (CBM). With decreasing metallicity and evolution along the TP phase, the He-shell flash and the t
Externí odkaz:
http://arxiv.org/abs/1510.07417
Autor:
Denissenkov, P., Truran, J. W., Herwig, F., Jones, S., Paxton, B., Nomoto, K., Suzuki, T., Toki, H.
When carbon is ignited off-centre in a CO core of a super-AGB star, its burning in a convective shell tends to propagate to the centre. Whether the C flame will actually be able to reach the centre depends on the efficiency of extra mixing beneath th
Externí odkaz:
http://arxiv.org/abs/1407.0248
Autor:
Denissenkov, Pavel A., Truran, James W., Pignatari, Marco, Trappitsch, Reto, Ritter, Christian, Herwig, Falk, Battino, Umberto, Setoodehnia, Kiana, Paxton, B.
Classical novae are the result of thermonuclear flashes of hydrogen accreted by CO or ONe white dwarfs, leading eventually to the dynamic ejection of the surface layers. These are observationally known to be enriched in heavy elements, such as C, O a
Externí odkaz:
http://arxiv.org/abs/1303.6265
Autor:
Stello, D., Huber, D., Bedding, T. R., Benomar, O., Bildsten, L., Elsworth, Y. P., Gilliland, R. L., Mosser, B., Paxton, B., White, T. R.
Of the more than 150000 targets followed by the Kepler Mission, about 10% were selected as red giants. Due to their high scientific value, in particular for Galaxy population studies and stellar structure and evolution, their Kepler light curves were
Externí odkaz:
http://arxiv.org/abs/1302.0858
We have computed an extensive grid of binary evolution tracks to represent low- and intermediate mass X-ray binaries (LMXBs and IMXBs). The grid includes 42,000 models which covers 60 initial donor masses over the range of 1-4 solar masses and, for e
Externí odkaz:
http://arxiv.org/abs/1012.1877
Autor:
Madhusudhan, N., Justham, S., Nelson, L., Paxton, B., Pfahl, E., Podsiadlowski, Ph., Rappaport, S.
Publikováno v:
Astrophys.J.640:918-922,2006
We have computed models for ultraluminous X-ray sources ("ULXs") consisting of a black-hole accretor of intermediate mass ("IMBH"; e.g., ~1000 Msun) and a captured donor star. For each of four different sets of initial donor masses and orbital separa
Externí odkaz:
http://arxiv.org/abs/astro-ph/0511393
Autor:
Albasri, A, Hattle, M, Koshiaris, C, Dunnington, A, Paxton, B, Fox, SE, Smith, M, Archer, L, Smith, KIE, Stevens, R, McManus, R, Sheppard, J
Objectives: There are many meta-analyses of randomised controlled trials (RCTs) which examine the efficacy of antihypertensive treatment, but few have studied the potential harms. The aim of this study was to examine the association between antihyper
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=od______1064::c9cd617d35b9faccf7eb968df701001f
https://ora.ox.ac.uk/objects/uuid:16daad7d-f9aa-4cbe-b986-85aca71c3f0a
https://ora.ox.ac.uk/objects/uuid:16daad7d-f9aa-4cbe-b986-85aca71c3f0a
Autor:
Jones, S., Hirschi, R., Nomoto, K., Fischer, T., Timmes, F. X., Herwig, F., Paxton, B., Toki, H., Suzuki, T., Martxednez-Pinedo, G., Lam, Y. H., Bertolli, M. G., Jones, Hirschi, Nomoto, Fischer, Timmes, F. X., Herwig, Paxton, Toki, Suzuki, Martxednez-Pinedo, Lam, Y. H., Bertolli, M. G.
Publikováno v:
The Astrophysical Journal.
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=erc_________::4dc7d2ae29eb0e5287d90d7bdfea413b
