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The Hamburg/RASS Catalogue of optical identifications. Northern high-galactic latitude ROSAT Bright Source Catalogue X-ray sources
We present the Hamburg/RASS Catalogue (HRC) of optical identificationsof X-ray sources at high-galactic latitude. The HRC includes all X-raysources from the ROSAT Bright Source Catalogue (RASS-BSC) with galacticlatitude |b| >=30degr and declination delta >=0degr . In thispart of the sky covering ~ 10 000 deg2 the RASS-BSC contains5341 X-ray sources. For the optical identification we used blue Schmidtprism and direct plates taken for the northern hemisphere Hamburg QuasarSurvey (HQS) which are now available in digitized form. The limitingmagnitudes are 18.5 and 20, respectively. For 82% of the selectedRASS-BSC an identification could be given. For the rest either nocounterpart was visible in the error circle or a plausibleidentification was not possible. With ~ 42% AGN represent the largestgroup of X-ray emitters, ~ 31% have a stellar counterpart, whereasgalaxies and cluster of galaxies comprise only ~ 4% and ~ 5%,respectively. In ~ 3% of the RASS-BSC sources no object was visible onour blue direct plates within 40\arcsec around the X-ray sourceposition. The catalogue is used as a source for the selection of(nearly) complete samples of the various classes of X-ray emitters.
| Speckle Interferometry at the U.S. Naval Observatory. XVII.
The results of 3362 intensified CCD observations of double stars, madewith the 26 inch refractor of the U.S. Naval Observatory, are presented.Each observation of a system represents a combination of over 2000short-exposure images. These observations are averaged into 1970 meanrelative positions and range in separation from 0farcs78 to 72farcs17,with a mean separation of 14farcs76. This is the 17th in this series ofpapers and covers the period 2010 January 6 through December 20. Alsopresented are 10 pairs that are resolved for the first time.
| New optical positions and proper motions of late type stars associated with SiO masers
The 33 cm astrograph of the Bordeaux Observatory has been used to derivewith respect to AGK3 reference stars, accurate positions of late typevariable stars variable stars associated with strong SiO maser emission.It is suggested that selected maser stars can be used to link theHIPPARCOS system and the VLBI extragalactic reference frame. The propermotions of the program (SiO) and reference stars are derived and, forthe program stars, are compared to the McCormick catalog of propermotions.
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| Takýmyýldýz: | Herkul |
| Sað Açýklýk: | 16h22m17.09s |
| Yükselim: | +18°32'02.0" |
| Görünürdeki Parlaklýk: | 10.748 |
| özdevim Sað Açýklýk: | -13.5 |
| özdevim Yükselim: | -23.5 |
| B-T magnitude: | 11.88 |
| V-T magnitude: | 10.842 |
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