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020 _a9781402038440
_99781402038440
024 7 _a10.1007/1402038445
_2doi
035 _avtls000334523
039 9 _a201509030211
_bVLOAD
_c201404120803
_dVLOAD
_c201404090543
_dVLOAD
_y201402041150
_zstaff
040 _aMX-SnUAN
_bspa
_cMX-SnUAN
_erda
050 4 _aQB1-991
100 1 _aCesarsky, Catherine.
_eeditor.
_9307016
245 1 0 _aISO Science Legacy :
_bA Compact Review of ISO Major Achievements /
_cedited by Catherine Cesarsky, Alberto Salama.
264 1 _aDordrecht :
_bSpringer Netherlands,
_c2005.
300 _avii, 446 páginas
_brecurso en línea.
336 _atexto
_btxt
_2rdacontent
337 _acomputadora
_bc
_2rdamedia
338 _arecurso en línea
_bcr
_2rdacarrier
347 _aarchivo de texto
_bPDF
_2rda
500 _aSpringer eBooks
505 0 _aGeneral -- Crystalline Silicates -- Water in Space: The Water World of ISO -- Molecular Hydrogen -- Understanding Galaxy Formation with ISO Deep Surveys -- Solar System -- The Planets and Titan Observed by ISO -- Comets, Asteroids and Zodiacal Light as Seen by Iso -- Stars and Circumstellar Matter -- ISO Observations of Pre-Stellar Cores and Young Stellar Objects -- Pre-Main Sequence Stars Seen by ISO -- Debris Discs Around Stars: The 2004 ISO Legacy -- Late Stages of Stellar Evolution -- Interstellar Medium -- The Cool Interstellar Medium -- High Excitation ISM and Gas -- The Ice Survey Opportunity of ISO -- Our Local Universe . . . -- Normal Nearby Galaxies -- Obscured Activity: AGN, Quasars, Starbursts and ULIGs Observed by the Infrared Space Observatory -- . . . And Beyond -- The European Large Area ISO Survey -- ISO’s Contribution to the Study of Clusters of Galaxies.
520 _aStars are born and die in clouds of gas and dust, opaque to most types of radiation, but transparent in the infrared. Requiring complex detectors, space missions and cooled telescopes, infrared astronomy is the last branch of this discipline to come of age. After a very successful sky survey performed in the eighties by the IRAS satellite, the Infrared Space Observatory, in the nineties, brought spectacular advances in the understanding of the processes giving rise to powerful infrared emission by a great variety of celestial sources. Outstanding results have been obtained on the bright comet Hale-Bopp, and in particular of its water spectrum, as well as on the formation, chemistry and dynamics of planetary objects in the solar system. Ideas on the early stages of stellar formation and on the stellar initial mass function have been clarified. ISO is the first facility in space able to provide a systematic diagnosis of the physical phenomena and the chemistry in the close environment of pre-main sequence stars, in the interstellar medium, and in the final stages of stellar life, using, among other indicators, molecular hydrogen, ubiquitous crystalline silicates, water and ices. ISO has dramatically increased our ability to investigate the power production, excitation and fuelling mechanism of galaxies of every type, and has discovered a new very cold dust component in galaxies. ISO has demonstrated that luminous infrared galaxies were brighter and much more numerous in the past, and that they played a dominant role in shaping present day galaxies and in producing the cosmic infrared background.
590 _aPara consulta fuera de la UANL se requiere clave de acceso remoto.
700 1 _aSalama, Alberto.
_eeditor.
_9307017
710 2 _aSpringerLink (Servicio en línea)
_9299170
776 0 8 _iEdición impresa:
_z9781402038433
856 4 0 _uhttp://remoto.dgb.uanl.mx/login?url=http://dx.doi.org/10.1007/1-4020-3844-5
_zConectar a Springer E-Books (Para consulta externa se requiere previa autentificación en Biblioteca Digital UANL)
942 _c14
999 _c281387
_d281387