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TYC 3825-180-1


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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

Stars with the Largest Hipparcos Photometric Amplitudes
A list of the 2027 stars that have the largest photometric amplitudes inHipparcos Photometry shows that most variable stars are all Miras. Thepercentage of variable types change as a function of amplitude. Thiscompilation should also be of value to photometrists looking forrelatively unstudied, but large amplitude stars.

New infrared carbon stars in the IRAS point source catalog.
We present new results of a search for infrared carbon stars (IRCS)based on the combination of IRAS and near infrared colours. A sample of207 stars with IRAS colours that characterize IRCS is selected andmeasured in the $JHKL$ photometric bands. Using a [12 - 25] vs. K - Lcolour diagram, 20 new IRCS candidates are proposed. Medium resolutionspectra in the ~ 6000-9000 Angstrom range of 8 of these candidatesconfirm their carbon rich nature. In addition we propose a few starswith LRS class "4n" as oxygen--rich candidates, and a few stars with LRSclasses "0n" and "1n" as carbon-rich. Based on observations obtained atthe Observatoire de Haute Provence, France. Tables 2 and 3 are onlyavailable in electronic form at the CDS via anonymous ftp tocdsarc.u-strasbg.fr (130.79.128.5) or viahttp://cdsweb.u-strasbg.fr/Abstract.html

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Datos observacionales y astrométricos

Constelación:Osa Mayor
Ascensión Recta:11h20m56.73s
Declinación:+54°49'58.3"
Magnitud Aparente:9.893
Movimiento Propio en Ascensión Recta:-1.4
Movimiento Propio en Declinación:-10.2
B-T magnitude:11.757
V-T magnitude:10.047

Catálogos y designaciones:
Nombres Propios   (Edit)
TYCHO-2 2000TYC 3825-180-1
USNO-A2.0USNO-A2 1425-07647985
HIPHIP 55417

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