... 000, 1­11 (2010) Printed 18 May 2010 A (MN L TEX style file v2.2) Magnetic field , chemical comp osition and line profile variability of the p eculiar eclipsing binary star AR Aur C.P. Folsom1 , O. Kochukhov2 , G.A. Wade3 , J. Silvester3,4 , S. Bagnulo1 1 2 3 4 Armagh Obs Department Department Department er ... However, the recent discovery of line profile variability in some HgMn stars, apparently attributable to surface abundance patches, has brought this belief into question. ...

Draft version September 5, 2005 A Preprint typ eset using L TEX style emulateap j v. 11/26/04 THE DEMOGRAPHICS OF LONG-PERIOD COMETS Paul J. Francis Research School of Astronomy and Astrophysics, the Australian National University, Mt STromlo Observatory, Cotter Road, Weston ACT 2611, Australia Draft version September 5, 2005 ABSTRACT The absolute magnitude and perihelion distributions of long-perio d comets are derived, using data from the Lincoln Near-Earth Asteroid Research (LINEAR) survey. ...

The Astrophysical Journal, 645:955 - 976, 2006 July 10 # 2006. The American Astronomical Society. All rights reserved. Printed in U.S.A. ChaMP SERENDIPITOUS GALAXY CLUSTER SURVEY W. A. Barkhouse, P. J. Green,1,2 A. Vikhlinin,2 D.-W. Kim,2 D. Perley,3 R. Cameron,4 J. Silverman,1,5 A. Mossman, R. Burenin,6 B. T. Jannuzi,7 M. Kim,2 M. G. Smith,8 R. C. Smith,8 H. Tananbaum,2 and B. J. Wilkes2 Received 2005 June 21; accepted 2006 March 19 1,2 2 ABSTRACT We present a survey of serendipitous extended X-ray sources

Jupiter on 2012-11-11 UT N W II I IV 1' Tag Name Jupiter I Io II Europa III Ganymede IV Callisto E 1 1 0 1 S 1 1 1 1 XEphem Jupiter View at 22:45:00 11/10/2012 EST, JD 2456242.65625 GRS in Sys II = 119.000; CML in Sys I = 62.820, in Sys II = 196.136 From Moore Observatory at Latitude 38:20:40 N Longitude 85:31:44 W Topocentric Astrometric 2000.00 Moon Positions, XYZ in Jupiter radii P T X +E Y +S Z +front RA 4:50:41.00 00 5.058 - ...