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HD 16419


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Hipparcos red stars in the HpV_T2 and V I_C systems
For Hipparcos M, S, and C spectral type stars, we provide calibratedinstantaneous (epoch) Cousins V - I color indices using newly derivedHpV_T2 photometry. Three new sets of ground-based Cousins V I data havebeen obtained for more than 170 carbon and red M giants. These datasetsin combination with the published sources of V I photometry served toobtain the calibration curves linking Hipparcos/Tycho Hp-V_T2 with theCousins V - I index. In total, 321 carbon stars and 4464 M- and S-typestars have new V - I indices. The standard error of the mean V - I isabout 0.1 mag or better down to Hp~9 although it deteriorates rapidly atfainter magnitudes. These V - I indices can be used to verify thepublished Hipparcos V - I color indices. Thus, we have identified ahandful of new cases where, instead of the real target, a random fieldstar has been observed. A considerable fraction of the DMSA/C and DMSA/Vsolutions for red stars appear not to be warranted. Most likely suchspurious solutions may originate from usage of a heavily biased color inthe astrometric processing.Based on observations from the Hipparcos astrometric satellite operatedby the European Space Agency (ESA 1997).}\fnmsep\thanks{Table 7 is onlyavailable in electronic form at the CDS via anonymous ftp tocdsarc.u-strasbg.fr (130.79.128.5) or viahttp://cdsweb.u-strasbg.fr/cgi-bin/qcat?J/A+A/397/997

High-velocity stars between the Magellanic Clouds
We report the positions of 12 new stars with high radial velocities(> 100 km s(-1) ) between the two Magellanic Clouds. These stars havebeen found using the Fehrenbach objective prism.

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Gözlemler ve gökölçümü verileri

Takýmyýldýz:Kucuk Su yilani
Sað Açýklýk:02h33m55.32s
Yükselim:-70°46'04.7"
Görünürdeki Parlaklýk:7.917
Uzaklýk:327.869 parsek
özdevim Sað Açýklýk:14.5
özdevim Yükselim:19
B-T magnitude:10.057
V-T magnitude:8.094

Kataloglar ve belirtme:
Özgün isimleri   (Edit)
HD 1989HD 16419
TYCHO-2 2000TYC 9147-1719-1
USNO-A2.0USNO-A2 0150-01337074
HIPHIP 11926

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