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We present spatial and spectral results of ROSAT observations of two galax-ies: NGC 4569 and NGC 4303. Both objects are members of the Virgo Cluster andhave nearby smaller companions with which they h...
The X-ray irradiated gas around a compact object was investigated. Wesolved the hydrostatic balance coupling with the ionization and thermal balancesto obtain the structure of the optically thin emiss...
X-ray line spectroscopy of massive x-ray binaries     X-ray line spectroscopy  x-ray binaries       font style='font-size:12px;'> 2009/6/4
Spectra from ASCA have provided the most detailed view to date of theX-ray spectral properties of stellar winds in massive X-ray binaries. Using de-tailed atomic mo dels that account for recombinat...
Coronal physics and the chandra emission line project      Coronal physics  LATE-TYPE       font style='font-size:12px;'> 2009/6/4
With the launch of the Chandra X-ray Observatory, high resolution X-rayspectroscopy of cosmic sources has begun. Early, deep observations of three stellarcoronal sources桟apella, Pro cyon, and HR 1099梐...
Hot gas and the gaseous structure of the galaxy     HYDRODYNAMICS  SUPERNOVAREMNANTS  X-RAYS  GALAXIES       font style='font-size:12px;'> 2009/6/4
A parochial review is presented concerning the status of our understandingof hot gas regions in the Galaxy and their implications for the overall distributionsof the Galaxy抯 gaseous components. We hav...
Needs and requirements for future x-ray observations of hot galactic halos     HALOS  X-RAYS  JETS AND OUTFLOWS       font style='font-size:12px;'> 2009/6/4
Galaxies are key objects for the study of cosmology, the life cycle of matter,and stellar evolution. X-ray observations have given us a new key window intothese building blocks of the Universe, that a...
Hot gas in the galaxy:what do we know for sure?      GENERAL GALAXY  BUBBLES ISM  GENERAL X-RAYS       font style='font-size:12px;'> 2009/6/4
Major advances have been made in the past decade in our knowledge of the hotinterstellar gas of our Milky Way galaxy. The Di.use X-ray Spectrometer obtainedspectra in the 0.15?.28 keV range from the G...
Coronal diagnostics     CORONA TECHNIQUES  X-RAYS  SPECTROSCOPIC ULTRAVIOLET       font style='font-size:12px;'> 2009/6/4
Ultraviolet emission line ratios have long provided powerful diagnostics for thedensity, temperature, elemental abundances and ionization state of astrophysicalplasmas. With the current generation of ...
Spectral measurement of Mkn 421 were made in the hard Xray energy band of 20–200 keV using a high sensitivity, large area scintillation counter telescope on November 21, 2000 and these coincided wit...
Soft X-ray Variability of the Bright Quasar 3C273      individual (3C273)  quasar—X-rays  galaxies       font style='font-size:12px;'> 2009/5/20
We present the results from ROSAT observations of 3C273 in the soft X-ray band. The light variation of 3C273 was investigated for three different energy bands of soft, medium, and hard. The maximum ...
Spectroscopic Studies of X-Ray Binary Pulsars      X-ray binaries  pulsars  spectra       font style='font-size:12px;'> 2009/5/19
Several new features of X-ray binary pulsars are revealed from recent observations with ASCA, RXTE, BeppoSAX and other Xray observatories. Among these, I will review in this paper some recent progr...
Photometric Variability of Four Coronally Active Stars     Stars variable  optical photometry  X-rays source       font style='font-size:12px;'> 2009/5/19
We present photometric observations of four stars that are optical counterparts of soft X-ray/EUV sources, namely 1ES 0829+15.9, 1ES0920-13.6, 2RE J110159+223509 and 1ES 1737+61.2. We have discovere...
We report the observation of nearest quasar 3C273 made with LASE instrument on November 20th, 1998 as a part of our continuing programme of balloon borne hard X-ray observations in the 20–200 keV b...
We present the results of a detailed analysis of RXTE observations of class ! (Klein-Wolt et al. 2002) which show an unusual state transition between high-soft and low-soft states in the Galactic mi...
The attempts at unified model fitting to explain the spectral variations in Cyg X-3 suggest equally probable fits with a combination of an absorbed blackbody and a separately absorbed power law with...

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