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HD 238698


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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 dwarf spheroidal galaxy in Draco. II. Galactic foreground reddening.
Abstract image available at:http://adsabs.harvard.edu/abs/1979AJ.....84.1167S

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Gözlemler ve gökölçümü verileri

Takýmyýldýz:Ejderha
Sað Açýklýk:17h26m41.69s
Yükselim:+59°44'55.6"
Görünürdeki Parlaklýk:9.705
özdevim Sað Açýklýk:2.3
özdevim Yükselim:-11.9
B-T magnitude:9.545
V-T magnitude:9.692

Kataloglar ve belirtme:
Özgün isimleri   (Edit)
HD 1989HD 238698
TYCHO-2 2000TYC 3900-447-1
USNO-A2.0USNO-A2 1425-08789289
HIPHIP 85374

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