000			02934nam a22004215i 4500
001			978-1-4020-4839-5
003			DE-He213
005			20251006084515.0
007			cr nn 008mamaa
008			100301s2006 ne | s |||| 0|eng d
020			_a9781402048395
020			_a99781402048395
024	7		_a10.1007/978-1-4020-4839-5 _2doi
082	0	4	_a520 _223
100	1		_aGómez de Castro, Ana I. _eeditor.
245	1	0	_aFundamental Questions in Astrophysics: Guidelines for Future UV Observatories _h[electronic resource] / _cedited by Ana I. Gómez de Castro, Willem Wamsteker.
264		1	_aDordrecht : _bSpringer Netherlands, _c2006.
300			_aIII, 170 p. _bonline resource.
336			_atext _btxt _2rdacontent
337			_acomputer _bc _2rdamedia
338			_aonline resource _bcr _2rdacarrier
347			_atext file _bPDF _2rda
505	0		_aStructure and Evolution of White Dwarfs and their Interaction with the Local Interstellar Medium -- Key Problems in Cool-Star Astrophysics -- UV Capabilities to Probe the Formation of Planetary Systems: From the ISM to Planets -- Ultraviolet Studies of Interacting Binaries -- The Need for Ultraviolet to Understand the Chemical Evolution of the Universe, and Cosmology -- Starbursts at Space Ultraviolet Wavelengths -- A View to the Future: Ultraviolet Studies of the Solar System -- Active Galaxies in the UV -- Fundamental Problems in Astrophysics -- Guidelines for Future UV Observatories -- Massive stars in the UV.
520			_aModern astrophysics is a mature science that has evolved from its early phase of discovery and classification to a physics-oriented discipline focused in finding answers to fundamental problems ranging from cosmology to the origin and diversity of life-sustainable systems in the Universe. For this very reason, progress of modern astrophysics requires the access to the electromagnetic spectrum in the broadest energy range. The Ultraviolet is a fundamental energy domain since it is one of the most powerful tool to study plasmas at temperatures in the 3,000-300,000~K range as well as electronic transitions of the most abundant molecules in the Universe. Moreover, the UV radiation field is a powerful astrochemical and photoionizing agent. This book describes the fundamental problems in modern astrophysics that cannot progress without easy and wide-spread access to modern UV instrumentation.
650		0	_aPHYSICS.
650		0	_aASTRONOMY.
650	1	4	_aPHYSICS.
650	2	4	_aASTRONOMY.
650	2	4	_aASTRONOMY, ASTROPHYSICS AND COSMOLOGY.
700	1		_aWamsteker, Willem. _eeditor.
710	2		_aSpringerLink (Online service)
773	0		_tSpringer eBooks
776	0	8	_iPrinted edition: _z9781402048388
856	4	0	_uhttp://dx.doi.org/10.1007/978-1-4020-4839-5 _zVer el texto completo en las instalaciones del CICY
912			_aZDB-2-PHA
942			_2ddc _cER
999			_c61029 _d61029