... The RAS Meteorite Collection: State on the 1 st of June, 1999 . ... About the laboratory . ... Find 1863. Several masses totaling 133 kg . ... Chondrite . ... Find 1873. One mass of 50 kg . ... Australia Union, Western Australia . Find 1963 or 1964. ... Australia Union, South Australia . Find 1972. ... Find 1973. ... Find 1955, racognized 1968. ... Find 1940. ... Find 1964. Several masses totaling more than 40 kg . ... Numerous masses totaling about 150 kg . ... Find 1947. ...

... FTP access the basic models is here . ... Below, we put short descriptions of the used SED models for the photometric redshifts providing by the current server . ... The uniqueness of this model consists in expanding to the near IR (NIR) of Rocca-Volmerange and Guiderdoni's (1988) atlas of synthetic spectra with a revised stellar library, which includes parameters of cool stars. ... Homepage of the GISSEL model). ... Another model used earlier is the model of synthetic spectra of Poggianti (1997). ...

Maria M. Katsova . I am a Leading Researcher in Stellar Astrophysics Department of SAI MSU . I began to work at Sternberg Astronomical Institute (SAI) in 1967, graduated from Moscow State University (MSU) in 1971, Ph.D.(MSU) since 1984. And now I become a Doctor of Sciences (Full Doctor of the Physical and Mathematical Sciences)(MSU, since 1999). ... I am a member of European Astronomical Society (EAS), Euro-Asian Astronomical Society (EAAS), National Geographic Society (NGS). ...

... Under certain conditions, like those in the nucleus of a QSO, all atoms can be made to emit light at particular wavelengths. ... If that source is approaching the observer, the wave is squashed up onto itself making the wavelength shorter. ... This is redshift. ... You can see how the section of the QSO spectrum which we observe changes with redshift. ... We then see how far we had to slide the observed spectrum along the scale to make it match and that is the objects redshift. ... The 2QZ team . ...

GCVS Variability Types and Distribution Statistics of Designated Variable Stars According to their Types of Variability ======================================================================== I. GCVS Variability Types. ... The new variability types (ZZO, AM, R, BE, LBV, BLBOO) have been added in the Name-Lists 67- 72 and in the GCVS vol.V. ZZO ZZ Cet type variables of the DO spectral type showing HeII and and CIV absorbtion lines in their spectra. ... RCB Variables of the R Coronae Borealis type. ...

... VaST is a software tool for finding variable objects on a series of astronomical images. ... VaST performs object detection and aperture photometry using SExtractor on each image, cross-matches lists of detected stars, performs magnitude calibration with respect to the first (reference) image and constructs a lightcurve for each object. ... VaST FITS image viewer ./pgfv . ... Part I" PZP, vol. ... K. V. Sokolovsky, S. A. Korotkiy; "New Variable Stars Discovered by the NMW Survey" PZP, vol. ...