Magnetic Stars, 2011, pp. 415 ­ 418 High Resolution Sp ectroscopy of the Star Feige 34 Han I.1 , Burlakova T.2 , Valyavin G.3 , Kim H. S.4 , Galazutdinov G.5 , Zharikov S. V.3 , Lee B.­C.1 , Kim K.­M.1 , Kholtygin We present high­resolution spectral observations of the hot subdwarf sdO star Feige 34. ... How did the giant progenitors of these stars loose their envelopes? ... 4 Discussion We have presented new high­resolution spectral observations of the hot sdO subdwarf star Feige 34. ...

CATS home ] [ Back to CATS list ] [ ftp ] . ... 117.1578Bock+ The Molonglo Observatory Synthesis Telescope, operating at 843 MHz with a 5 deg^2 field of view, is carrying out a radio imaging survey of the sky south of declination -30 deg. This survey (the Sydney University Molonglo Sky Survey, or SUMSS) produces images with a resolution of 43"x43" csc|delta| and an rms noise level of ~1 mJy beam^-1. ... See also MGPS2 Galactic plane survey. ...

... Bogod V.M., Gel'freikh G.B.: Study of the solar atmosphere based on spectral and polarization observations on the RATAN-600. ... V.M. Bogod, C. Mercier, L. V. Yasnov: About the nature of long-term microflare energy release in the solar active regions, Paper accepted by JGR in 2000 (Manuscript Number: 20.4013). ... Bogod V.M., Garaimov V., Grebinskij A., Komar N., Opeikina L.: Solar active regions study based on wide wavelength range radio observations with RATAN-600, Abstract of JENAM-2000, p.115 . ...

... Corresponding gates in each row are connected in parallel at both edges of the array. ... Other gates. ... otherwise indicated, 45 kpixels/sec and standard voltages using a dual slope CDS circuit (8 µs integration time) Minimum Format Pixel Size Imaging Area Dark current (MPP), 20° C equivalent Readout noise Front Back Full Well signal Output gain CTE per pixel Typical 512 x 512 pixels 24 µm x 24 µm 12.3 mm x 12.3 mm 50 pa/cm2 5 electrons 7 electrons 350,000 electrons 1.5 µV/ electron 0 ...