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A minimal timescale for the continuum in 4U 1608-52 and Aql X-1

Mohamed, K.; Sonbas, E.; Dhuga, K. S.; Gogus, E.; Tuncer, A.; Abd Allah, N. N.; Ibrahim, A.


Dublin Core

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<oai_dc:dc xmlns:dc="http://purl.org/dc/elements/1.1/" xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xsi:schemaLocation="http://www.openarchives.org/OAI/2.0/oai_dc/ http://www.openarchives.org/OAI/2.0/oai_dc.xsd">
  <dc:creator>Mohamed, K.</dc:creator>
  <dc:creator>Sonbas, E.</dc:creator>
  <dc:creator>Dhuga, K. S.</dc:creator>
  <dc:creator>Gogus, E.</dc:creator>
  <dc:creator>Tuncer, A.</dc:creator>
  <dc:creator>Abd Allah, N. N.</dc:creator>
  <dc:creator>Ibrahim, A.</dc:creator>
  <dc:date>2021-01-01</dc:date>
  <dc:description>Similar to black hole X-ray binary transients, hysteresis-like state transitions are also seen in some neutron-star X-ray binaries. Using a method based on wavelets and light curves constructed from archival Rossi X-ray Timing Explorer observations, we extract a minimal timescale over the complete range of transitions for 4U 1608-52 during the 2002 and 2007 outbursts and the 1999 and 2000 outbursts for Aql X-1. We present evidence for a strong positive correlation between this minimal timescale and a similar timescale extracted from the corresponding power spectra of these sources.</dc:description>
  <dc:identifier>https://aperta.ulakbim.gov.trrecord/231404</dc:identifier>
  <dc:identifier>oai:aperta.ulakbim.gov.tr:231404</dc:identifier>
  <dc:rights>info:eu-repo/semantics/openAccess</dc:rights>
  <dc:rights>http://www.opendefinition.org/licenses/cc-by</dc:rights>
  <dc:source>MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY 502(1) L72-L78</dc:source>
  <dc:title>A minimal timescale for the continuum in 4U 1608-52 and Aql X-1</dc:title>
  <dc:type>info:eu-repo/semantics/article</dc:type>
  <dc:type>publication-article</dc:type>
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