Zobrazeno 1 - 10
of 22
pro vyhledávání: '"Herbert H. B. Lau"'
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 437:195-214
We have computed detailed evolution and nucleosynthesis models for super and massive AGB stars over the mass range 6.5-9.0 Msun in divisions of 0.5 Msun with metallicities Z=0.02, 0.008 and 0.004. These calculations, in which we find third dredge-up
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::c70a971c5b380da2c4d7b46cce6fc36b
https://doi.org/10.1093/mnras/stt1877
https://doi.org/10.1093/mnras/stt1877
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 435:698-706
Certain carbon-enhanced metal-poor stars likely obtained their composition via pollution from some of the earliest generations of asymptotic giant branch stars and as such provide important clues to early Universe nucleosynthesis. Recently, Kinman et
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::219d011d53675d1fabac1fe3089ce9ba
https://doi.org/10.1093/mnras/stt1329
https://doi.org/10.1093/mnras/stt1329
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 415:959-963
Models of rapidly rotating massive stars at low metallicities show significantly different evolution and higher metal yields compared to non-rotating stars. We estimate the spin-down time-scale of rapid rotating non-convective stars supporting an alp
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::095907eed835f8387bc86544ca0577c5
https://doi.org/10.1111/j.1365-2966.2011.18766.x
https://doi.org/10.1111/j.1365-2966.2011.18766.x
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 410:2458-2462
The stellar origin of gamma-ray bursts can be explained by the rapid release of energy in a highly collimated, extremely relativistic jet. This in turn appears to require a rapidly spinning highly magnetised stellar core that collapses into a magneti
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::a9be1dc2a8f598a0c6688ae710e0d5f4
https://doi.org/10.1111/j.1365-2966.2010.17622.x
https://doi.org/10.1111/j.1365-2966.2010.17622.x
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 385:301-309
We use the Cambridge stellar evolution code STARS to model the evolution of 5-7 solar mass zero-metallicity stars. With enhanced resolution at the hydrogen and helium burning shell in the AGB phases, we are able to model the entire thermally pulsing
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::08ca556256035ebbd65196933dac85c7
https://doi.org/10.1111/j.1365-2966.2007.12816.x
https://doi.org/10.1111/j.1365-2966.2007.12816.x
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 378:563-568
We use the Cambridge stellar evolution code STARS to model the evolution and nucleosynthesis of zero-metallicity intermediate-mass stars. We investigate the effect of duplicity on the nucleosynthesis output of these systems and the potential abundanc
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::26cb720c1fc7669eeccd6a365108ccc7
https://doi.org/10.1111/j.1365-2966.2007.11773.x
https://doi.org/10.1111/j.1365-2966.2007.11773.x
Autor:
Richard J. Stancliffe, Simon Campbell, Carolyn Doherty, Ilka Petermann, M. Lugaro, Herbert H. B. Lau
Publikováno v:
Proceedings of XIII Nuclei in the Cosmos — PoS(NIC XIII).
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::da06cc3df63a65f18fb2eb4dfbff8189
https://doi.org/10.22323/1.204.0089
https://doi.org/10.22323/1.204.0089
The origin of the stellar initial mass function (IMF) is a fundamental issue in the theory of star formation. It is generally fit with a composite power law. Some clues on the progenitors can be found in dense starless cores that have a core mass fun
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::7143d3c5db698bea382fd52e3916a5ac
Autor:
Christopher A. Tout, Robert G. Izzard, Ross P. Church, Herbert H. B. Lau, Carolyn Doherty, Anna N. Żytkow
The very bright red star HV2112 in the Small Magellanic Cloud could be a massive Thorne-Zytkow Object, a supergiant-like star with a degenerate neutron core. With its luminosity of over $10^5\,\rm L_\odot$, it could also be a super asymptotic giant b
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::cb9779a57b05f6a3616831ea9e7708c1
http://arxiv.org/abs/1406.6064
http://arxiv.org/abs/1406.6064
Autor:
John C. Lattanzio, Pilar Gil-Pons, Herbert H. B. Lau, Simon Campbell, Carolyn Doherty, Lionel Siess
Publikováno v:
Recercat. Dipósit de la Recerca de Catalunya
Universitat Jaume I
Monthly notices of the Royal Astronomical Society, 441 (1
UPCommons. Portal del coneixement obert de la UPC
Universitat Politècnica de Catalunya (UPC)
Universitat Jaume I
Monthly notices of the Royal Astronomical Society, 441 (1
UPCommons. Portal del coneixement obert de la UPC
Universitat Politècnica de Catalunya (UPC)
We present a new grid of stellar models and nucleosynthetic yields for super-AGB stars with metallicities Z = 0.001 and 0.0001, applicable for use within galactic chemical evolution models. Contrary to more metal-rich stars where hot bottom burning i
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::de89af4c3c6c31cf40c369e87d74e509
https://hdl.handle.net/2117/27588
https://hdl.handle.net/2117/27588