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HD 154183


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관련 글

The Wolf 630 moving group of stars
An analysis is made of the probability of collective membership of thestars assigned by Eggen to the Wolf 630 moving group. This probabilityis estimated from the scatter of points in the color-absolute magnitudediagram when compared to the intrinsic scatter observed for M67.Particular attention is paid to the random errors for all the observedand deduced stellar parameters. Results show that either theobservational errors must be about 2.4 times larger than given in theproper motion and radial velocity source catalogues, or the intrinsicscatter in the color-magnitude diagram for the Wolf 630 group must bemuch larger than for M67, or many of the stars considered cannot bemembers.

Stellar Groups in the Old Disk Population
Not Available

Colors, luminosities, and motions of the nearer G-type stars
Abstract image available at:http://adsabs.harvard.edu/cgi-bin/nph-bib_query?1964AJ.....69..570E&db_key=AST

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관측 및 측정 데이터

별자리:헤르쿨레스자리
적경:17h02m55.21s
적위:+25°38'19.8"
가시등급:8.674
거리:111.111 파섹
적경상의 고유운동:-34.5
적위상의 고유운동:-122.7
B-T magnitude:9.463
V-T magnitude:8.74

천체목록:
일반명   (Edit)
HD 1989HD 154183
TYCHO-2 2000TYC 2064-277-1
USNO-A2.0USNO-A2 1125-07968544
HIPHIP 83412

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