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HD 148327


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Ýlgili Makaleler

Astrometric and astrophysical discontinuities between the galactic old disk and halo stellar populations
Intermediate band, RI, and DDO photometry of the weak-lined stars in thefirst three volumes of the Michigan catalogs of spectral type arediscussed on the basis of luminosity and heavy element abundance. Theinterface between the old disk (Fe/H greater than -0.8 dex) and halo(Fe/H less than -1.2 dex) populations represents discontinuities in boththe stellar motions and the stellar physics. The CN strengths of bothevolved and unevolved halo stars decrease with decreasing temperature,in a mirror image of the increase with decreasing temperature for thedisk objects. The result for the halo giants has been attributed to deepmixing in the stellar atmospheres but the similar result for unevolveddwarfs indicates a difference in formation rather than in evolutionaryprocess of the two populations.

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Gözlemler ve gökölçümü verileri

Takýmyýldýz:Guney Ucgeni
Sað Açýklýk:16h32m02.56s
Yükselim:-67°17'40.7"
Görünürdeki Parlaklýk:8.564
Uzaklýk:303.951 parsek
özdevim Sað Açýklýk:5.4
özdevim Yükselim:-34.9
B-T magnitude:9.553
V-T magnitude:8.646

Kataloglar ve belirtme:
Özgün isimleri   (Edit)
HD 1989HD 148327
TYCHO-2 2000TYC 9049-277-1
USNO-A2.0USNO-A2 0225-25595391
HIPHIP 80970

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