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HD 49246


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An Einstein Observatory SAO-based catalog of B-type stars
About 4000 X-ray images obtained with the Einstein Observatory are usedto measure the 0.16-4.0 keV emission from 1545 B-type SAO stars fallingin the about 10 percent of the sky surveyed with the IPC. Seventy-fourdetected X-ray sources with B-type stars are identified, and it isestimated that no more than 15 can be misidentified. Upper limits to theX-ray emission of the remaining stars are presented. In addition tosummarizing the X-ray measurements and giving other relevant opticaldata, the present extensive catalog discusses the reduction process andanalyzes selection effects associated with both SAO catalog completenessand IPC target selection procedures. It is concluded that X-rayemission, at the level of Lx not less than 10 exp 30 ergs/s, is quitecommon in B stars of early spectral types (B0-B3), regardless ofluminosity class, but that emission, at the same level, becomes lesscommon, or nonexistent, in later B-type stars.

The classification of intrinsic variable stars. II. The red variables of S and related types
Abstract image available at:http://adsabs.harvard.edu/cgi-bin/nph-bib_query?1972ApJ...177..489E&db_key=AST

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观测天体数据

星座:麒麟座
右阿森松:06h47m46.55s
赤纬:+06°17'49.1"
视星:7.918
距离:1369.863 天文距离
右阿森松适当运动:0.3
赤纬适当运动:1.2
B-T magnitude:7.841
V-T magnitude:7.912

目录:
适当名称
HD 1989HD 49246
TYCHO-2 2000TYC 160-788-1
USNO-A2.0USNO-A2 0900-03535729
HIPHIP 32569

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