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001			280412
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008			150903s2007 xxu| o |||| 0|eng d
020			_a9780387682884 _99780387682884
024	7		_a10.1007/9780387682884 _2doi
035			_avtls000331846
039		9	_a201509030214 _bVLOAD _c201404121938 _dVLOAD _c201404091705 _dVLOAD _y201402041014 _zstaff
040			_aMX-SnUAN _bspa _cMX-SnUAN _erda
050		4	_aQB1-991
100	1		_aRobinson, Keith. _eautor _9305318
245	1	0	_aSpectroscopy: The Key to the Stars : _bReading the Lines in Stellar Spectra / _cby Keith Robinson.
264		1	_aNew York, NY : _bSpringer New York, _c2007.
300			_axii, 160 páginas _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		_aPatrick Moore’s Practical Astronomy Series, _x1431-9756
500			_aSpringer eBooks
505	0		_aSpectroscopy—A New Golden Age for Amateur Astronomy -- The Basic Stuff—Light Radiation and Atoms -- Behind the Lines—The Magnificent Energy Level Structure of an Atom -- Our Old Friend the Doppler Effect -- When Is a Spectral Line Not a Spectral Line? -- Stellar Spectra and That Famous Mnemonic -- Cool but not Smooth—The Molecular Spectra of Red Stars -- Glows in the Dark—Emission Lines and Nebulae -- Glowing Vortices—Accretion Disks -- The P Cygni Profile and Friends -- Spectral Magnetism—The Zeeman Effect -- ‘How Much Gold in Them There Stars?’—The Curve of Growth.
520			_aMore can be learned about physical processes going on in stars and nebulae by understanding and analyzing their spectra than by any other means. Many amateur astronomers who use CCD cameras are taking up spectroscopy as part of their observational program, but until now the physics that underlies astronomical spectroscopy has been confined to advanced academic books. Not any more! In Spectroscopy – the Key to the Stars, Keith Robinson describes the physics and physical processes that cause the stellar spectra to be as they are… spectra that amateur astronomers can image with today’s commercially-made equipment. Written specifically for amateur astronomers, this book assumes only a basic knowledge of physics but looks in detail at many topics, including energy levels in atoms, the molecular spectra of red stars, emission lines in nebulae, and much, much more. Here is everything you need to know about how the atomic processes in stars and nebulae produce the spectra that amateur astronomers can image, and why spectroscopy is such a powerful tool for astronomers.
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: _z9780387367866
856	4	0	_uhttp://remoto.dgb.uanl.mx/login?url=http://dx.doi.org/10.1007/978-0-387-68288-4 _zConectar a Springer E-Books (Para consulta externa se requiere previa autentificación en Biblioteca Digital UANL)
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999			_c280412 _d280412