Zobrazeno 1 - 10
of 65
pro vyhledávání: '"Fenner, Yeshe"'
Autor:
Fenner, Yeshe, Garland, Suzanne M, Moore, Elya E, Jayasinghe, Yasmin, Fletcher, Ashley, Tabrizi, Sepehr N, Gunasekaran, Bharathy, Wark, John D
Publikováno v:
Journal of Medical Internet Research, Vol 14, Iss 1, p e20 (2012)
BackgroundRecruitment of young people for health research by traditional methods has become more expensive and challenging over recent decades. The Internet presents an opportunity for innovative recruitment modalities. ObjectiveTo assess the feasib
Externí odkaz:
https://doaj.org/article/347051e352014b119d367e561bb2e40a
Autor:
Bailes, Matthew, McClelland, David, Thrane, Eric, Blair, David, Cooke, Jeffrey, Coward, David, Evans, Robin, Fenner, Yeshe, Galloway, Duncan, Hurley, Jarrod, Ju, Li, Lasky, Paul, Mandel, Ilya, McKenzie, Kirk, Melatos, Andrew, Ottaway, David, Scott, Susan, Slagmolen, Bram, Veitch, Peter, Wen, Linqing, Zhao, Chunnong
The past four years have seen a scientific revolution through the birth of a new field: gravitational-wave astronomy. The first detection of gravitational waves---recognised by the 2017 Nobel Prize in Physics---provided unprecedented tests of general
Externí odkaz:
http://arxiv.org/abs/1912.06305
Autor:
Fenner, Yeshe.
Publikováno v:
Connect to this title online.
Thesis (Ph. D.)--Swinburne University of Technology, 2005.
Title from PDF title page (viewed on *). Includes bibliographical references.
Title from PDF title page (viewed on *). Includes bibliographical references.
Externí odkaz:
http://adt.lib.swin.edu.au/public/adt-VSWT20050804.161449/
This thesis explores the chemical signatures of galaxy formation and evolution using a software package designed specifically for this investigation. We describe the development of this multi-zone chemical evolution code, which simulates the spacetim
Externí odkaz:
http://adt.lib.swin.edu.au./public/adt-VSWT20050804.161449
[abridged]We calculate multi-wavelength spectral energy distributions (SEDs) (spanning optical to millimeter wavelengths) from simulations of major galaxy mergers with black hole feedback which produce submillimeter bright galaxies (SMGs), using a se
Externí odkaz:
http://arxiv.org/abs/astro-ph/0610860
Publikováno v:
Astrophys.J.652:1240-1245,2006
We investigate the suggestion that there are stellar populations in some globular clusters with enhanced helium (Y from 0.28 to 0.40) compared to the primordial value. We assume that a previous generation of massive Asymptotic Giant Branch (AGB) star
Externí odkaz:
http://arxiv.org/abs/astro-ph/0608366
Using a chemical evolution model we investigate the intriguing suggestion that there are populations of stars in some globular clusters (e.g. NGC 2808, omega Centauri) with enhanced levels of helium (Y from about 0.28 to 0.40) compared to the majorit
Externí odkaz:
http://arxiv.org/abs/astro-ph/0605540
Publikováno v:
Astrophys.J. 646 (2006) 184-191
The chemical properties of dwarf spheroidals in the local group are shown to be inconsistent with star formation being truncated after the reionization epoch (z~8). Enhanced levels of [Ba/Y] in stars in dwarf spheroidals like Sculptor indicate strong
Externí odkaz:
http://arxiv.org/abs/astro-ph/0602489
Publikováno v:
Mon.Not.Roy.Astron.Soc. 356 (2005) 1071-1078
The chemical evolution history of a galaxy hides clues about how it formed and has been changing through time. We have studied the chemical evolution history of the Milky Way (MW) and Andromeda (M31) to find which are common features in the chemical
Externí odkaz:
http://arxiv.org/abs/astro-ph/0410579
Publikováno v:
Astrophys.J. 606 (2004) 116-125
We have investigated chemical evolution in the young universe by analysing the detailed chemical enrichment pattern of a metal-rich galaxy at high redshift. The recent detection of over 20 elements in the gas-phase of a damped Lyman-alpha absorber (D
Externí odkaz:
http://arxiv.org/abs/astro-ph/0401413