The real-time stellar evolution of Sakurai's object

Science

Volumn 308, Issue 5719, 2005, Pages 231-233

  Hajduk, Marcin ^a,b   Zijlstra, Albert A ^a   Herwig, Falk ^c   Van Hoof, Peter A M ^d,e   Kerber, Florian ^f   Kimeswenger, Stefan ^g   Pollacco, Don L ^d   Evans, Aneurin ^h   Lopéz, José A ⁱ   Bryce, Myfanwy ^a   Eyres, Stewart P S ^j   Matsuura, Mikako ^a  

^a UNIVERSITY OF MANCHESTER   (United Kingdom)

^b NICOLAUS COPERNICUS UNIVERSITY   (Poland)

^c LOS ALAMOS NATIONAL LABORATORY   (United States)

^d QUEEN'S UNIVERSITY BELFAST   (United Kingdom)

^e ROYAL OBSERVATORY OF BELGIUM   (Belgium)

^f EUROPEAN SOUTHERN OBSERVATORY   (Germany)

^g UNIVERSITY OF INNSBRUCK   (Austria)

^h KEELE UNIVERSITY   (United Kingdom)

ⁱ UNIVERSIDAD NACIONAL AUTÓNOMA DE MÉXICO   (Mexico)

^j UNIVERSITY OF CENTRAL LANCASHIRE   (United Kingdom)

more..

Author keywords

[No Author keywords available]

Indexed keywords

CARBON; COMBUSTION; DUST; HEAT CONVECTION; HEATING; IONIZATION; MIXING; THERMAL EFFECTS;

CARBONACEOUS DUST; DWARF; RADIO EMISSION; SAKURAI'SO BJECT;

GALAXIES;

CARBON; HELIUM; HYDROGEN; NITROGEN; OXYGEN;

ASTRONOMY;

ARTICLE; ASTRONOMY; COMPUTER SIMULATION; COSMOLOGICAL PHENOMENA; ELECTRON; HEATING; IONIZATION; LUMINANCE; MASS; PRIORITY JOURNAL; STAR; TEMPERATURE;

EID: 20244366547     PISSN: 00368075     EISSN: None     Source Type: Journal    
DOI: 10.1126/science.1108953     Document Type: Article

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30. Supported by the EU Marie Curie Training Site program under contract HPMT-CT-2000-00069 (M.H.), Los Alamos National Laboratory under U.S. Department of Energy contract W-7405-ENC-36 (F.H.), the UK Engineering and Physical Sciences Research Council (P.A.M.V.H.), the UK Particle Physics and Astronomy Research Council (M.M.), an extended-visit grant to the UK from the Royal Society and the Academia Mexicana de Ciencias (J.A.L), and the Nuffield Foundation (S.P.S.E.). The photoionization code Cloudy can be obtained from www.nublado.org. The observations described above made use of the Very Large Array, operated by the National Radio Astronomy Observatory, and the ESO Very Large Telescope.