A search for X-rays from five pulsars: PSR's 0740-28, 1737-30, 1822-09, 1915+13 and 1916+14

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dc.creatorAlpar, M. A.
dc.creatorGuseinov, O. H.
dc.creatorKiziloglu, U.
dc.creatorOgelman, H.
dc.date1995-03-11
dc.date.accessioned2026-07-07T06:27:55Z
dc.date.available2026-07-07T06:27:55Z
dc.descriptionWe report observations of PSR's 0740-28, 1737-30, 1822-09, 1915+13 and 1916+14 with ROSAT. In the 0.1-2.1 keV range upper limits to luminosity are derived for power law and blackbody spectra, using a range of $N_{H}$ estimates. The upper limit to the blackbody luminosity from PSR1822-09 turns out to be consistent with standard cooling curves. For the other pulsars the upper limits are not restrictive as they are much larger than the luminosities predicted by the models.
dc.descriptionuuencoded compressed postscript, 4 pages including figures, to be published by A&A
dc.identifierhttps://arxiv.org/abs/astro-ph/9503049
dc.identifierhttp://arxiv.org/abs/astro-ph/9503049
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/97556
dc.subjectAstrophysics
dc.titleA search for X-rays from five pulsars: PSR's 0740-28, 1737-30, 1822-09, 1915+13 and 1916+14
dc.typetext

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