Ultraviolet emission from young and middle-aged pulsars: Connecting X-rays with the optical

Oleg Kargaltsev, George Pavlov

Research output: Contribution to journalArticle

22 Citations (Scopus)

Abstract

We present the UV spectroscopy and timing of three nearby pulsars (Vela, B0656+14 and Geminga) recently observed with the Space Telescope Imaging Spectrograph. We also review the optical and X-ray properties of these pulsars and establish their connection with the UV properties. We show that the multiwavelengths properties of neutron stars (NSs) vary significantly within the sample of middle-aged pulsars. Even larger differences are found between the thermal components of Geminga and B0656+14 as compared to those of radio-quiet isolated NSs. These differences could be attributed to different properties of the NS surface layers.

Original languageEnglish (US)
Pages (from-to)287-296
Number of pages10
JournalAstrophysics and Space Science
Volume308
Issue number1-4
DOIs
StatePublished - Apr 1 2007

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ultraviolet emission
pulsars
surface layer
spectroscopy
radio
neutron stars
x rays
spectrographs
surface layers
time measurement
telescopes
young

All Science Journal Classification (ASJC) codes

  • Astronomy and Astrophysics
  • Space and Planetary Science

Cite this

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Ultraviolet emission from young and middle-aged pulsars : Connecting X-rays with the optical. / Kargaltsev, Oleg; Pavlov, George.

In: Astrophysics and Space Science, Vol. 308, No. 1-4, 01.04.2007, p. 287-296.

Research output: Contribution to journalArticle

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