The ASCA catalog of potential X-ray counterparts of GeV sources

Mallory Roberts, Roger W. Romani, Nobuyuki Kawai

    Research output: Contribution to journalArticle

    Abstract

    We present a catalog of 2-10 keV ASCA Gas Imaging Spectrometer images of fields containing bright sources of GeV emission. The images cover ~ 85% of the 95% confidence position contour for 28 of the 30 sources with > 1 GeV fluxes above 4 × 10-8 ph cm-2 s-1. We find an excess of hard X-ray sources with F2-10keV ≳ 10-12 ergs cm-2 s-1 positionally coincident with unidentified sources of GeV emission. We comment on radio-loud and radio-quiet pulsar candidates, as well as several SNRs and massive binaries as possible sources of the GeV emission. We also find evidence for a class of variable γ-ray sources associated with extended regions of hard X-ray emission, and propose that for these sources, a significant percentage of the γ-ray emission is generated in synchrotron nebulae surrounding fast, young pulsars.

    Original languageEnglish (US)
    Pages (from-to)451-465
    Number of pages15
    JournalAstrophysical Journal, Supplement Series
    Volume133
    Issue number2
    DOIs
    StatePublished - Apr 1 2001

    Fingerprint

    catalogs
    x rays
    radio
    pulsars
    rays
    erg
    spectrometer
    imaging spectrometers
    nebulae
    confidence
    synchrotrons
    gas
    gases

    Keywords

    • Gamma rays: observations
    • Pulsars: general
    • Stars: Wolf-Rayet
    • Supernova remnants
    • X-rays

    ASJC Scopus subject areas

    • Space and Planetary Science

    Cite this

    The ASCA catalog of potential X-ray counterparts of GeV sources. / Roberts, Mallory; Romani, Roger W.; Kawai, Nobuyuki.

    In: Astrophysical Journal, Supplement Series, Vol. 133, No. 2, 01.04.2001, p. 451-465.

    Research output: Contribution to journalArticle

    Roberts, Mallory ; Romani, Roger W. ; Kawai, Nobuyuki. / The ASCA catalog of potential X-ray counterparts of GeV sources. In: Astrophysical Journal, Supplement Series. 2001 ; Vol. 133, No. 2. pp. 451-465.
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