Skip to main content

6 Result(s)

within Conference Paper Remove this filter S Kitamoto Remove this filter

and

  1. No Access

    Chapter and Conference Paper

    X-ray Observation of Black Hole Novae

    X-ray novae are the best objects to study their compact stars. Some of the X-ray novae have been confirmed that they were containing a black hole based on dynamical mass estimations. Besides the dynamical mass...

    S. Kitamoto in Observational Evidence for Black Holes in the Universe (1999)

  2. No Access

    Chapter and Conference Paper

    Direct Measurement of the CCD with a Subpixel Resolution by Using a New Technique

    The response function of the front-illuminated CCD, like SIS on ASCA, can be devided into three parts: the gate structure transmission, the absorption efficiency in the depletion region and the charge spreadin...

    K. Yoshita, S. Kitamoto, E. Miyata, H. Tsunemi, K. C. Gendreau in The Hot Universe (1998)

  3. No Access

    Chapter and Conference Paper

    X-Ray Determination of the Black-Hole Mass in Cygnus X-1

    About 10 X-ray binaries in our Galaxy and LMC/SMC are considered to contain black hole candidates (BHCs). Among these objects, Cyg X-l was identified as the first BHC, and it has led BHCs for more than 25 year...

    A. Kubota, K. Makishima, T. Dotani, H. Inoue, K. Mitsuda, F. Nagase… in The Hot Universe (1998)

  4. No Access

    Chapter and Conference Paper

    The Circumstellar Matter of Cygnus X-3

    X-ray source in Cyg X-3 is embedded in the photo-ionized circumstellar gas. Recombination edges and emission lines were detected by ASCA observation (Kawashima, Kitamoto 1996; Liedahl, Paerels 1996). The stren...

    S. Kitamoto, K. Kawashima in The Hot Universe (1998)

  5. No Access

    Chapter and Conference Paper

    Chemical Abundances of Early Type Stars

    X-rays from early-type stars are emitted by the corona or the stellar wind. The materials in the surface layer of early-type stars are not contaminated by nuclear reactions in the stellar inside. Therefore, ab...

    S. Tanaka, S. Kitamoto, T. Suzuki, K. Torii, M. F. Corcoran, W. Waldron in The Hot Universe (1998)

  6. No Access

    Chapter and Conference Paper

    Temperature Profiles of Accretion Disks in X-Ray Binaries

    We present the new results of fitting X-ray spectra of two representative X-ray binaries; X-ray Nova Muscae 1991 and Cyg X-2, by a non-steady disk model, in which a temperature gradient, a ≡ — dlogT/dlogr, is lef...

    S. Mineshige, F. Honma, A. Hirano, S. Kitamoto, T. Yamada… in Theory of Accretion Disks — 2 (1994)