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HD 189721


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Ýlgili Makaleler

Two-colour photometry for 9473 components of close Hipparcos double and multiple stars
Using observations obtained with the Tycho instrument of the ESAHipparcos satellite, a two-colour photometry is produced for componentsof more than 7 000 Hipparcos double and multiple stars with angularseparations 0.1 to 2.5 arcsec. We publish 9473 components of 5173systems with separations above 0.3 arcsec. The majority of them did nothave Tycho photometry in the Hipparcos catalogue. The magnitudes arederived in the Tycho B_T and V_T passbands, similar to the Johnsonpassbands. Photometrically resolved components of the binaries withstatistically significant trigonometric parallaxes can be put on an HRdiagram, the majority of them for the first time. Based on observationsmade with the ESA Hipparcos satellite.

Photographic observations of visual double stars
Photographic observations of 238 pairs of visual binaries obtained on770 plates using the 60-cm visual refractor of Bosscha Observatory(Lembang, Java) during 1976-1979 are reported, continuing the catalog ofvan Albada-van Dien (1983). The data-reduction procedures are brieflydescribed, and the data are presented in a table.

Photographic observations of visual double stars
Mean positions, the corresponding epochs, relative separations, positionangles, and mean errors are presented for 95 pairs of visual doublestars, mostly in the Southern Hemisphere. The results were obtained bymeasuring plates taken with the 60-cm visual refractor of BosschaObservatory, Lembang, Indonesia, over a 16-yr period. The reductionmethod used in determining the mean positions, epochs, and errors isdiscussed.

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Gözlemler ve gökölçümü verileri

Takýmyýldýz:Tavus
Sað Açýklýk:20h05m08.77s
Yükselim:-63°03'41.7"
Görünürdeki Parlaklýk:7.721
Uzaklýk:178.891 parsek
özdevim Sað Açýklýk:13.1
özdevim Yükselim:-36.7
B-T magnitude:7.848
V-T magnitude:7.732

Kataloglar ve belirtme:
Özgün isimleri
HD 1989HD 189721
TYCHO-2 2000TYC 9090-1312-1
USNO-A2.0USNO-A2 0225-30530234
HIPHIP 98919

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