<?xml version="1.0" encoding="UTF-8"?>
<collection xmlns="http://www.loc.gov/MARC21/slim">
 <record>
  <leader>     caa a22        4500</leader>
  <controlfield tag="001">469077271</controlfield>
  <controlfield tag="003">CHVBK</controlfield>
  <controlfield tag="005">20180323132938.0</controlfield>
  <controlfield tag="007">cr unu---uuuuu</controlfield>
  <controlfield tag="008">170328e19920901xx      s     000 0 eng  </controlfield>
  <datafield tag="024" ind1="7" ind2="0">
   <subfield code="a">10.1007/BF02507857</subfield>
   <subfield code="2">doi</subfield>
  </datafield>
  <datafield tag="035" ind1=" " ind2=" ">
   <subfield code="a">(NATIONALLICENCE)springer-10.1007/BF02507857</subfield>
  </datafield>
  <datafield tag="245" ind1="0" ind2="0">
   <subfield code="a">X-ray signatures of cold accretion disks in AGNs</subfield>
   <subfield code="h">[Elektronische Daten]</subfield>
   <subfield code="c">[G. Matt, G. Perola, L. Piro]</subfield>
  </datafield>
  <datafield tag="520" ind1="3" ind2=" ">
   <subfield code="a">Summary: We have calculated, by means of Monte Carlo simulations, the properties of the radiation emerging from an X-ray illuminated cold accretion disk. These calculations can apply to AGNs, for which there is evidence of cold, optically thick matter near the central black hole. The resulting spectra show an intense iron fluorescent line and a high-energy bump above about 10 keV, where the scattering becomes important with respect to the photoabsorption; these features have been observed by GINGA in some bright Seyfert 1 galaxies. Our detailed results are indicative of the type of future observations which would lead to estimates of the geometrical parameters of the disk, its iron abundance and the mass of the black hole.</subfield>
  </datafield>
  <datafield tag="540" ind1=" " ind2=" ">
   <subfield code="a">Società Italiana di Fisica, 1992</subfield>
  </datafield>
  <datafield tag="690" ind1=" " ind2="7">
   <subfield code="a">X-ray sources</subfield>
   <subfield code="2">nationallicence</subfield>
  </datafield>
  <datafield tag="700" ind1="1" ind2=" ">
   <subfield code="a">Matt</subfield>
   <subfield code="D">G.</subfield>
   <subfield code="u">Istituto Astronomico, Università «La Sapienza», Via G. Lancisi 29, 00161, Roma, Italia</subfield>
   <subfield code="4">aut</subfield>
  </datafield>
  <datafield tag="700" ind1="1" ind2=" ">
   <subfield code="a">Perola</subfield>
   <subfield code="D">G.</subfield>
   <subfield code="u">Istituto Astronomico, Università «La Sapienza», Via G. Lancisi 29, 00161, Roma, Italia</subfield>
   <subfield code="4">aut</subfield>
  </datafield>
  <datafield tag="700" ind1="1" ind2=" ">
   <subfield code="a">Piro</subfield>
   <subfield code="D">L.</subfield>
   <subfield code="u">Istituto di Astrofisica Spaziale, CNR, Via E. Fermi 23, 00044, Frascati, Italia</subfield>
   <subfield code="4">aut</subfield>
  </datafield>
  <datafield tag="773" ind1="0" ind2=" ">
   <subfield code="t">Il Nuovo Cimento C</subfield>
   <subfield code="d">Kluwer Academic Publishers</subfield>
   <subfield code="g">15/5(1992-09-01), 825-829</subfield>
   <subfield code="x">0390-5551</subfield>
   <subfield code="q">15:5&lt;825</subfield>
   <subfield code="1">1992</subfield>
   <subfield code="2">15</subfield>
   <subfield code="o">11543</subfield>
  </datafield>
  <datafield tag="856" ind1="4" ind2="0">
   <subfield code="u">https://doi.org/10.1007/BF02507857</subfield>
   <subfield code="q">text/html</subfield>
   <subfield code="z">Onlinezugriff via DOI</subfield>
  </datafield>
  <datafield tag="908" ind1=" " ind2=" ">
   <subfield code="D">1</subfield>
   <subfield code="a">research-article</subfield>
   <subfield code="2">jats</subfield>
  </datafield>
  <datafield tag="950" ind1=" " ind2=" ">
   <subfield code="B">NATIONALLICENCE</subfield>
   <subfield code="P">856</subfield>
   <subfield code="E">40</subfield>
   <subfield code="u">https://doi.org/10.1007/BF02507857</subfield>
   <subfield code="q">text/html</subfield>
   <subfield code="z">Onlinezugriff via DOI</subfield>
  </datafield>
  <datafield tag="950" ind1=" " ind2=" ">
   <subfield code="B">NATIONALLICENCE</subfield>
   <subfield code="P">700</subfield>
   <subfield code="E">1-</subfield>
   <subfield code="a">Matt</subfield>
   <subfield code="D">G.</subfield>
   <subfield code="u">Istituto Astronomico, Università «La Sapienza», Via G. Lancisi 29, 00161, Roma, Italia</subfield>
   <subfield code="4">aut</subfield>
  </datafield>
  <datafield tag="950" ind1=" " ind2=" ">
   <subfield code="B">NATIONALLICENCE</subfield>
   <subfield code="P">700</subfield>
   <subfield code="E">1-</subfield>
   <subfield code="a">Perola</subfield>
   <subfield code="D">G.</subfield>
   <subfield code="u">Istituto Astronomico, Università «La Sapienza», Via G. Lancisi 29, 00161, Roma, Italia</subfield>
   <subfield code="4">aut</subfield>
  </datafield>
  <datafield tag="950" ind1=" " ind2=" ">
   <subfield code="B">NATIONALLICENCE</subfield>
   <subfield code="P">700</subfield>
   <subfield code="E">1-</subfield>
   <subfield code="a">Piro</subfield>
   <subfield code="D">L.</subfield>
   <subfield code="u">Istituto di Astrofisica Spaziale, CNR, Via E. Fermi 23, 00044, Frascati, Italia</subfield>
   <subfield code="4">aut</subfield>
  </datafield>
  <datafield tag="950" ind1=" " ind2=" ">
   <subfield code="B">NATIONALLICENCE</subfield>
   <subfield code="P">773</subfield>
   <subfield code="E">0-</subfield>
   <subfield code="t">Il Nuovo Cimento C</subfield>
   <subfield code="d">Kluwer Academic Publishers</subfield>
   <subfield code="g">15/5(1992-09-01), 825-829</subfield>
   <subfield code="x">0390-5551</subfield>
   <subfield code="q">15:5&lt;825</subfield>
   <subfield code="1">1992</subfield>
   <subfield code="2">15</subfield>
   <subfield code="o">11543</subfield>
  </datafield>
  <datafield tag="900" ind1=" " ind2="7">
   <subfield code="a">Metadata rights reserved</subfield>
   <subfield code="b">Springer special CC-BY-NC licence</subfield>
   <subfield code="2">nationallicence</subfield>
  </datafield>
  <datafield tag="898" ind1=" " ind2=" ">
   <subfield code="a">BK010053</subfield>
   <subfield code="b">XK010053</subfield>
   <subfield code="c">XK010000</subfield>
  </datafield>
  <datafield tag="949" ind1=" " ind2=" ">
   <subfield code="B">NATIONALLICENCE</subfield>
   <subfield code="F">NATIONALLICENCE</subfield>
   <subfield code="b">NL-springer</subfield>
  </datafield>
 </record>
</collection>
