X­RAY STUDY OF CRAB­LIKE AND COMPOSITE SNRS K. TORII, H. TSUNEMI Osaka University AND P. SLANE Harvard­Smithsonian Center for Astrophysics 1. ... We have observed several objects including 3C58, CTA1, and G292.0+1.8. ... 1997; Torii et al. 1997). ... Al­ though the center­filled radio morphology suggested an interior plerionic component, strong X­ray emission lines seemed to rule out such specula­ tions. ... G292.0+1.8 0.5 ­ 2 keV G292.0+1.8 2 ­ 10 keV Figure 1. ASCA SIS images of G292.0+1.8. ...

Full-Text Search . ... arXiv.org . astro-ph . ... SAI VO . Search sort results by Date Relevance . Use logical operators AND , OR , NOT and round brackets to construct complex queries. Whitespace-separated words are treated as AND ed. Show 10 50 100 articles per page in Full Compact mode . Normalized to: Hasuike, K. 1 article(s) in total . 5 co-authors. Median position in authors list is 3,0 . Co-author(s): . ... Astronet | SAI MSU . ...

Next: Optical light curves Up: xnov Previous: xnov . ... Optical light curves . B light curve (Shugarov, 1976) . UBV light curves (Lyutyi, 1976) . UBV light curves (van den Bergh, 1976) . UBV light curves (Duerbeck and Walter, 1976) . B light curve (Lloyd et al., 1977) . ... B light curve (Robertson et al., 1976) . B-V data (Robertson et al., ... B' data (Tsunemi et al. ... X-ray light curves . 3-6 keV light curve (Kaluzienski et al. ...

... Future seminars . P a s t seminars . Seminar council . X-ray observation of middle-aged SNRs " . Prof. Hiroshi Tsunemi (Graduate School of Science, Earth and Space Science Osaka University) . ... We have studied the Cygnus Loop, a typical middle-aged SNR, in X-ray using the Asca and Rosat satellites. ... The shell region, high density region, shows a abundance of the ISM while the inner region, low density region, shows a metal rich abundance originating from the ejecta. ...

... Flux density at 1 GHz (/Jy): 210 . ... Optical: Large filamentary loop, brightest to the NE, not well defined to the S or W. X-ray: Shell in soft X-rays. ... DRAO at 408 MHz (3'.3?6'.7) for spectral index study, plus X-ray and optical. ADS . ... Optical spectroscopy of nearside filaments. ... 1992, ApJ, 400, 214. ... IRAS observations. ... Leahy et al. ... Far-UV spectroscopy, H and other optical observations of NE region. ... Suzaku observations of NE. ... Suzaku observations of N. ADS . ...

... We present status reports on projects to make both raw data and products from the Ginga X-ray astronomy satellite available in FITS formats to the general astronomical community. ... In parallel with the data reformatting project, a database of software products (light curves and spectra) is being produced at Leicester University which will also be made widely available. ... In parallel with creating hypercube format data products, the output routines are being rewritten to write FITS files as well....

... Here we present and discuss Vela Jr. properties revealed by these multiwavelength observations, and confront them with the SNR model expectations. ... Multiple observations of Vela Jr. in the radio band confirmed the shell-like structure and supported the identification of RX J0852.0-4622 as a SNR [8,11,12,13,14,16,46]. ... The X-ray emission line feature at 4.2 keV found by ASCA [48] in the NW rim spectrum of RX J0852.0-4622 was confirmed by XMM-Newton data (Fig. 4, 5, and [22]), and by Chandra [4]...

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... The dispersed spectrum shows a series of monochromatic images of the source in the light of individual spectral lines. ... Images formed in the light of strong X-ray emission lines are labeled. ... The dispersed images of prominent lines from the MEG ю1 order are shown with a uniform spatial scale and 2 pixel Gaussian smoothing in Figure 4. ... Distortions of the SNR ring shape can be seen by comparing the ring from the Ne x Ly line (Fig. 4, middle right panel ) with the undispersed image of Figure...

BD Bonner Durchmusterung, F.W.A. Argelander, Bonner Sternverzeichniss, 1 bis 4 sektion, Astronomische Beobachtungen auf der Sternwarte de Kgl. Rhein/ Friedrich-Wilhelms-Unviersiaet zu Bonn (CDS Cat. I/122). CoD Cordoba Durchmusterung, J. M. Thome, Resultados del Observatorio Nacional Argentino 16 - 18; 21, 1892-1932 (CDS Cat. I/114). CPD Cape Photographic Durchmusterung, D. GIll and J. C. Kapteyn, Ann. Cape Obs. 3-5, 1895 - 1900 (CDS Cat. I/108). DM Durchmusterungen. GSC B. M. Lasker, C. R. Sturch, B. J.

Асланов А.А., Хрузина Т.С. О периодической переменности оптического блеска V471 Tau вне затмения. Aстрон. журнал, 1988, 65 , 188-193 (Sov.Astr., ... Бочкарев Н.Г., Сюняев Р.А., Хрузина Т.С., Черепащук А.М., Шакура Н.И. Анизотропия излучения аккреционного диска вокруг черной дыры, прогрев оптической компоненты и орбитальные параметры двойной системы LMC X-3. ... Хрузина Т.С., Черепащук А.М. Интерпретация фотографической затменной кривой блеска HZ Her в неактивном состоянии. ...

... 0.00e+00 . ... 3d6(5D)4s a6D . ... 3d6(3F2)4s b4F . ... 3d6(3P2)4s b4P . ... 3d7 a4F . ... 3d6(3H)4s a4H . ... 3d7 a4P . ... 3d6(3D)4s b4D . ... 3d6(5D)4s a4D . ... 3d6(5D)4p z4Fo . ... 3d6(3F1)4s c4F . ... 3d6(5D)4p z4Do . ... 3d6(3P1)4s c4P . ... 3d6(5D)4p z4Po . ...

... 4 Горбацкий В.Г. Введение в физику галактик и скоплений галактик. ... 8 Freeman K.C. On the disks of spiral and SO galaxies. ApJ, 1970, v. 160, p. 811-830. ... Nearby Galaxies. ... AsAp, 1987, v. 173, p. 59-80. ... 15 Robin A.C., Oblak E. A kinematic model of the galaxy. -- 10 th European regional Astronomy meeting of the IAU, Praha, August 24-29, 1987, p. 323-326. ... ApJ. ... 75 Dather M., Biermann P.L. Accretion in disk galaxies: the hydrodynamical evolution of molecular rings. ...

Dynamics and Statistics M/M 10 4 statistics R = 0.9992 2 103 dynamics R = 0.9401 10 2 2 log(/o) -1.8 -1.7 -1.6 -1.5 -1.4 -1.3 -1.2 -1.1 -1 Comparison of results of mass estimation which is received by means of our method (dynamics) for 18 clusters of Milky Way with suspected BH with data in [2] (Safonova, Shastri, Aph. ... We considered the limits of central bodies masses for 4 clusters in our Galaxy (47 Tuc, Cen, NGC 6388, M15) and G1 Globular cluster in the Galaxy Andromeda. ...

... Deviations from the previously published wavelength calibration are less than 1 pixel (40 е) for the +1st order over nearly the entire field. ... j8eu07qbq j8eu07qcq j8eu07qdq j8eu07qeq j8eua6sxq j8eua6syq j8eua6szq j8eua6t0q j8eua6t3q j8eua6t4q j8eua7qlq j8eua7qmq j8eua7qnq WR96 WR96 WR96 WR96 WR96 WR96 WR96 WR96 WR96 WR96 WR96 WR96 WR96 WR96 WR96 WR96 WR96 WR96 WR96 WR96 WR96 WR96 WR96 WR96 WR96 WR96 WR96 WR96 WR96 F775W G800L ...