000 03114nam a22003855i 4500
001 288740
003 MX-SnUAN
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007 cr nn 008mamaa
008 150903s2012 xxu| o |||| 0|eng d
020 _a9781461422754
_99781461422754
024 7 _a10.1007/9781461422754
_2doi
035 _avtls000340832
039 9 _a201509030351
_bVLOAD
_c201404300421
_dVLOAD
_y201402061035
_zstaff
040 _aMX-SnUAN
_bspa
_cMX-SnUAN
_erda
050 4 _aQB1-991
100 1 _aDavidson, Kris.
_eeditor.
_9318638
245 1 0 _aEta Carinae and the Supernova Impostors /
_cedited by Kris Davidson, Roberta M. Humphreys.
264 1 _aBoston, MA :
_bSpringer US,
_c2012.
300 _ax, 329 páginas 88 ilustraciones, 31 ilustraciones en color.
_brecurso en línea.
336 _atexto
_btxt
_2rdacontent
337 _acomputadora
_bc
_2rdamedia
338 _arecurso en línea
_bcr
_2rdacarrier
347 _aarchivo de texto
_bPDF
_2rda
490 0 _aAstrophysics and Space Science Library,
_x0067-0057 ;
_v384
500 _aSpringer eBooks
505 0 _aEta Carinae - From 1600 to the Present -- The Company Eta Carinae Keeps - Stellar and Interstellar Content of the Carina -- The Central Star - Instability and Recovery -- The Winds of Eta Carinae and Other Very Luminous Stars -- Physics of the Inner Ejecta -- High-resolution Studies of Eta Carinae's Ejecta and Stellar Wind -- All Things Homunculus -- The Outer Ejecta -- X-ray Variability and the Secondary Star -- Eta Carinae and the Luminous Blue Variables -- The Supernova Imposters -- Instability and Mass Loss Near the Eddington Limit -- The Final Struggles of Massive Star Evolution and Their Supernovae.
520 _aIn 1965 Fritz Zwicky proposed a class of supernovae that he called "Type V", described as "excessively faint at maximum." There were only two members, SN1961v and eta Carinae. We now know that eta Carinae was not a true supernova, but if it were observed today in a distant galaxy we would call it a "supernova impostor." 170 years ago it experienced a "great eruption" lasting 20 years, expelling 10 solar masses or more, and survived. Eta Carinae is now acknowledged as the most massive, most luminous star in our region of the Galaxy, and it may be our only accessible example of a very massive star in a pre-supernova state. In this book the editors and contributing authors review its remarkable history, physical state of the star and its ejecta, and its continuing instability. Chapters also include its relation to other massive, unstable stars, the massive star progenitors of supernovae, and the "first" stars in the Universe.
590 _aPara consulta fuera de la UANL se requiere clave de acceso remoto.
700 1 _aHumphreys, Roberta M.
_eeditor.
_9318639
710 2 _aSpringerLink (Servicio en línea)
_9299170
776 0 8 _iEdición impresa:
_z9781461422747
856 4 0 _uhttp://remoto.dgb.uanl.mx/login?url=http://dx.doi.org/10.1007/978-1-4614-2275-4
_zConectar a Springer E-Books (Para consulta externa se requiere previa autentificación en Biblioteca Digital UANL)
942 _c14
999 _c288740
_d288740