000			03308nam a22004455i 4500
001			978-0-387-09691-9
003			DE-He213
005			20260521091821.0
007			cr nn 008mamaa
008			110402s2009 xxu| s |||| 0|eng d
020			_a9780387096919
020			_a99780387096919
024	7		_a10.1007/978-0-387-09691-9 _2doi
040			_cCICY
100	1		_aGordon, M.A. _eauthor.
245	1	0	_aRadio Recombination Lines _h[recurso electrónico] : _bTheir Physics and Astronomical Applications / _cby M.A. Gordon, R.L. Sorochenko.
264		1	_aNew York, NY : _bSpringer New York, _c2009.
300			_aXVI, 360p. 110 illus. _bonline resource.
336			_atext _btxt _2rdacontent
337			_acomputer _bc _2rdamedia
338			_arecurso en línea _bcr _2rdacarrier
347			_atext file _bPDF _2rda
490	1		_aAstrophysics and Space Science Library, _x0067-0057 ; _v282
505	0		_aRRLs and Atomic Physics -- RRLs: Tools for Astronomers -- Constants -- Tables of Line Frequencies -- Supplemental Calculations -- Hydrogen Oscillator Strengths -- Departure Coefficients -- Observational Units.
520			_aRadio Recombination Lines is a comprehensive guide to the physics and observations of Radio Recombination Lines from astronomical sources. It includes the history of RRL detections, the astrophysics underlying their intensities and line shapes including topics like departures from LTE and Stark broadening, the maximum possible size of an atom, as well as detailed descriptions of the astronomical topics for which RRLs have proved to be effective tools. In addition, the appendix includes detailed physics underlying the Bohr atomic model, tables of RRL frequencies including fine structure components, techniques for calculating hydrogenic oscillator strengths, and formulas for converting telescope intensity units to astrophysical ones. Radio Recombination Lines is written for astronomers and physicists. It is also suitable as a graduate-level textbook. This softcover contains updates and corrections from the previous hardcover published in 2002. "We now have a splendid book written by two of the pioneers, M.A. Gordon of the National Radio Astronomy Observatory in Tucson and R.L. Sorochenko of the Lebedev Institute. In their Preface the authors say that the book was written by exchanging email. They give a fascinating account of the history of the subject, a detailed discussion of the atomic physics required for the interpretation of the observations, and describe astronomical results obtained using RRL observations for a wide range of astronomical objects." -Mike Seaton, Former President, Royal Astronomical Society, 1979-1981
650		0	_aPHYSICS.
650		0	_aASTRONOMY.
650		0	_aMOLECULAR STRUCTURE.
650	1	4	_aPHYSICS.
650	2	4	_aASTRONOMY.
650	2	4	_aATOMIC AND MOLECULAR STRUCTURE AND SPECTRA.
700	1		_aSorochenko, R.L. _eauthor.
710	2		_aSpringerLink (Online service)
773	0		_tSpringer eBooks
776	0	8	_iPrinted edition: _z9780387096049
830		0	_aAstrophysics and Space Science Library, _x0067-0057 ; _v282
856	4	0	_uhttp://dx.doi.org/10.1007/978-0-387-09691-9 _zVer el texto completo en las instalaciones del CICY
942			_2ddc _cER
999			_c31966 _d31966