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007			cr nn 008mamaa
008			150903s2012 xxu| o |||| 0|eng d
020			_a9781441984449 _99781441984449
024	7		_a10.1007/9781441984449 _2doi
035			_avtls000339241
039		9	_a201509030315 _bVLOAD _c201404300357 _dVLOAD _y201402060930 _zstaff
040			_aMX-SnUAN _bspa _cMX-SnUAN _erda
050		4	_aQC1-75
100	1		_aMiller, Steve. _eautor _9316716
245	1	4	_aThe Chemical Cosmos : _bA Guided Tour / _cby Steve Miller.
264		1	_aNew York, NY : _bSpringer New York, _c2012.
300			_axii, 236 páginas 25 ilustraciones, 22 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		_aAstronomers' Universe, _x1614-659X
500			_aSpringer eBooks
505	0		_aPrologue -- Purple haze: introducing our guide -- The early universe: the source of chemistry – and of our guide -- Shooting the rapids: the life, and death, of the earliest starlight -- Interlude - how our guide is hooked, lost and caught again -- Heading downstream and cooking by starlight -- Fishing for molecules -- Branching out: in the land of the giants and dwarves -- Interlude - trawling for our cosmic guide -- In the delta: exoplanets - worlds, but not as we know them -- Towards the sea of life -- Epilogue -- Annotated references and further reading to chapters -- Some useful numbers -- Index.
520			_aIf you have ever wondered how we get from the awesome impersonality of the Big Bang universe to the point where living creatures can start to form, and evolve into beings like you, your friends and your family, wonder no more. Steve Miller provides us with a tour through the chemical evolution of the universe, from the formation of the first molecules all the way to the chemicals required for life to evolve. Using a simple Hydrogen molecule – known as H-three-plus - as a guide, he takes us on a journey that starts with the birth of the first stars, and how, in dying, they pour their hearts out into enriching the universe in which we live. Our molecular guide makes its first appearance at the source of the Chemical Cosmos, at a time when only three elements and a total of 11 molecules existed. From those simple beginnings, H-three-plus guides us down river on the violent currents of exploding stars, through the streams of the Interstellar Medium, and into the delta where new stars and planets form. We are finally left on the shores of the sea of life. Along the way, we meet the key characters who have shaped our understanding of the chemistry of the universe, such as Cambridge physicist J.J. Thomson and the Chicago chemist Takeshi Oka. And we are given an insider’s view of just how astronomers, making use of telescopes and Earth-orbiting satellites, have put together our modern view of the Chemical Cosmos.
590			_aPara consulta fuera de la UANL se requiere clave de acceso remoto.
710	2		_aSpringerLink (Servicio en línea) _9299170
776	0	8	_iEdición impresa: _z9781441984432
856	4	0	_uhttp://remoto.dgb.uanl.mx/login?url=http://dx.doi.org/10.1007/978-1-4419-8444-9 _zConectar a Springer E-Books (Para consulta externa se requiere previa autentificación en Biblioteca Digital UANL)
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999			_c287507 _d287507