03359nam a22004455i 4500001001800000003000900018005001700027007001500044008004100059020001800100020001900118024003500137040000900172100002600181245013800207264004600345300004400391336002600435337002600461338003900487347002400526490006200550505021400612520155200826650001302378650001502391650002502406650001302431650001502444650004802459700003002507710003402537773002002571776003602591830006202627856010302689942001202792999001702804952009202821978-0-387-09691-9DE-He21320260521091821.0cr nn 008mamaa110402s2009    xxu|    s    |||| 0|eng d  a9780387096919  a997803870969197 a10.1007/978-0-387-09691-92doi  cCICY1 aGordon, M.A.eauthor.10aRadio Recombination Linesh[recurso electrónico] :bTheir Physics and Astronomical Applications /cby M.A. Gordon, R.L. Sorochenko. 1aNew York, NY :bSpringer New York,c2009.  aXVI, 360p. 110 illus.bonline resource.  atextbtxt2rdacontent  acomputerbc2rdamedia  arecurso en líneabcr2rdacarrier  atext filebPDF2rda1 aAstrophysics and Space Science Library,x0067-0057 ;v2820 aRRLs and Atomic Physics -- RRLs: Tools for Astronomers -- Constants -- Tables of Line Frequencies -- Supplemental Calculations -- Hydrogen Oscillator Strengths -- Departure Coefficients -- Observational Units.  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 0aPHYSICS. 0aASTRONOMY. 0aMOLECULAR STRUCTURE.14aPHYSICS.24aASTRONOMY.24aATOMIC AND MOLECULAR STRUCTURE AND SPECTRA.1 aSorochenko, R.L.eauthor.2 aSpringerLink (Online service)0 tSpringer eBooks08iPrinted edition:z9780387096049 0aAstrophysics and Space Science Library,x0067-0057 ;v28240uhttp://dx.doi.org/10.1007/978-0-387-09691-9zVer el texto completo en las instalaciones del CICY  2ddccER  c31966d31966  00102ddc40708LEaCICYbCICYcELd2025-07-10l0r2025-07-10 08:39:24w2025-07-10yER