LEADER 01162nam a22002771i 4500 001 991002913829707536 005 20030817171308.0 008 030925s1980 sw |||||||||||||||||fre 020 $a9122003738 035 $ab1235434x-39ule_inst 035 $aARCHE-040188$9ExL 040 $aBiblioteca Interfacoltà$bita$cA.t.i. Arché s.c.r.l. Pandora Sicilia s.r.l. 082 04$a445 100 1 $aBartning, Inge$0455028 245 10$aRemarques sur la syntaxe et la sémantique des pseudo-adjectifs dénominaux en français /$cInge Bartnin 250 $a2. ed. 260 $aStockholm :$bAlmqvist & Wiksell international,$c1980 300 $a174 p. ;$c23 cm 440 0$aActa universitatis stockholmiensis.$pRomanica stockholmiensia ;$v10 650 4$aLingua francese$xAggettivi 907 $a.b1235434x$b02-04-14$c08-10-03 912 $a991002913829707536 945 $aLE002 D Ann. 177/010$g1$i2002000179463$lle002$o-$pE0.00$q-$rl$s- $t0$u0$v0$w0$x0$y.i12758528$z08-10-03 996 $aRemarques sur la syntaxe et la sémantique des pseudo-adjectifs dénominaux en français$9158120 997 $aUNISALENTO 998 $ale002$b08-10-03$cm$da $e-$ffre$gsw $h0$i1 LEADER 03086nam 22005295 450 001 9910254577303321 005 20200702091426.0 010 $a981-10-4524-0 024 7 $a10.1007/978-981-10-4524-0 035 $a(CKB)4340000000061884 035 $a(DE-He213)978-981-10-4524-0 035 $a(MiAaPQ)EBC6312181 035 $a(MiAaPQ)EBC5579414 035 $a(Au-PeEL)EBL5579414 035 $a(OCoLC)1066193044 035 $a(PPN)202989232 035 $a(EXLCZ)994340000000061884 100 $a20170601d2017 u| 0 101 0 $aeng 135 $aurnn|008mamaa 181 $ctxt$2rdacontent 182 $cc$2rdamedia 183 $acr$2rdacarrier 200 10$aBlack Holes: A Laboratory for Testing Strong Gravity /$fby Cosimo Bambi 205 $a1st ed. 2017. 210 1$aSingapore :$cSpringer Singapore :$cImprint: Springer,$d2017. 215 $a1 online resource (XV, 340 p. 123 illus., 117 illus. in color.) 311 $a981-10-4523-2 327 $aIntroduction -- Black Hole Solutions -- Motion around Black Holes -- Astrophysical Black Holes -- Thin Accretion Disks -- Thermal Spectrum of Thin Disks -- Relativistic Iron Line -- Quasi-Periodic Oscillations -- Parametrization of the Background Metric -- Observational Constraints. 330 $aThis textbook introduces the current astrophysical observations of black holes, and discusses the leading techniques to study the strong gravity region around these objects with electromagnetic radiation. More importantly, it provides the basic tools for writing an astrophysical code and testing the Kerr paradigm. Astrophysical black holes are an ideal laboratory for testing strong gravity. According to general relativity, the spacetime geometry around these objects should be well described by the Kerr solution. The electromagnetic radiation emitted by the gas in the inner part of the accretion disk can probe the metric of the strong gravity region and test the Kerr black hole hypothesis. With exercises and examples in each chapter, as well as calculations and analytical details in the appendix, the book is especially useful to the beginners or graduate students who are familiar with general relativity while they do not have any background in astronomy or astrophysics. 606 $aAstrophysics 606 $aGravitation 606 $aAstrophysics and Astroparticles$3https://scigraph.springernature.com/ontologies/product-market-codes/P22022 606 $aClassical and Quantum Gravitation, Relativity Theory$3https://scigraph.springernature.com/ontologies/product-market-codes/P19070 615 0$aAstrophysics. 615 0$aGravitation. 615 14$aAstrophysics and Astroparticles. 615 24$aClassical and Quantum Gravitation, Relativity Theory. 676 $a523.8875 700 $aBambi$b Cosimo$4aut$4http://id.loc.gov/vocabulary/relators/aut$0799778 801 0$bMiAaPQ 801 1$bMiAaPQ 801 2$bMiAaPQ 906 $aBOOK 912 $a9910254577303321 996 $aBlack Holes: a Laboratory for Testing Strong Gravity$91835293 997 $aUNINA