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HD 221037


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Absolute proper motions of open clusters. I. Observational data
Mean proper motions and parallaxes of 205 open clusters were determinedfrom their member stars found in the Hipparcos Catalogue. 360 clusterswere searched for possible members, excluding nearby clusters withdistances D < 200 pc. Members were selected using ground basedinformation (photometry, radial velocity, proper motion, distance fromthe cluster centre) and information provided by Hipparcos (propermotion, parallax). Altogether 630 certain and 100 possible members werefound. A comparison of the Hipparcos parallaxes with photometricdistances of open clusters shows good agreement. The Hipparcos dataconfirm or reject the membership of several Cepheids in the studiedclusters. Tables 1 and 2 are only available in electronic form at theCDS via anonymous ftp to cdsarc.u-strasbg.fr (130.79.128.5) or viahttp://cdsweb.u-strasbg.fr/Abstract.html

Observations in regions of Cassiopeia, Gemini, and Monoceros with the Glazar space telescope
Observations at 1640 A of regions in Cassiopeia, Gemini, and Monocerosmade with the Glazar space telescope are presented; 7, 11, 13, and 35early-type stars brighter than about 9 mag were detected in the observedregions. The distribution of dust matter in the corresponding regions isstudied. It is determined that companions of HD 4442, 4797, and BD + 62deg 2225 are subdwarfs of sdB - sdO types; the hot companion of HD220102 may be of the type from B8 Ib-II to sdB. It is shown that HD 5233and 261490 are probably embedded in dense circumstellar envelopes.

Etude cinematique et photometrique d'une region de Cas.
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Datos observacionales y astrométricos

Constelación:Casiopea
Ascensión Recta:23h28m05.82s
Declinación:+61°55'13.2"
Magnitud Aparente:8.102
Distancia:293.255 parsecs
Movimiento Propio en Ascensión Recta:12.1
Movimiento Propio en Declinación:-2
B-T magnitude:8.089
V-T magnitude:8.101

Catálogos y designaciones:
Nombres Propios   (Edit)
HD 1989HD 221037
TYCHO-2 2000TYC 4284-794-1
USNO-A2.0USNO-A2 1500-09784459
HIPHIP 115841

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