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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
| New periodic variables from the Hipparcos epoch photometry
Two selection statistics are used to extract new candidate periodicvariables from the epoch photometry of the Hipparcos catalogue. Theprimary selection criterion is a signal-to-noise ratio. The dependenceof this statistic on the number of observations is calibrated usingabout 30000 randomly permuted Hipparcos data sets. A significance levelof 0.1 per cent is used to extract a first batch of candidate variables.The second criterion requires that the optimal frequency be unaffectedif the data are de-trended by low-order polynomials. We find 2675 newcandidate periodic variables, of which the majority (2082) are from theHipparcos`unsolved' variables. Potential problems with theinterpretation of the data (e.g. aliasing) are discussed.
| The 74th Special Name-list of Variable Stars
We present the Name-list introducing GCVS names for 3153 variable starsdiscovered by the Hipparcos mission.
| Classification and Identification of IRAS Sources with Low-Resolution Spectra
IRAS low-resolution spectra were extracted for 11,224 IRAS sources.These spectra were classified into astrophysical classes, based on thepresence of emission and absorption features and on the shape of thecontinuum. Counterparts of these IRAS sources in existing optical andinfrared catalogs are identified, and their optical spectral types arelisted if they are known. The correlations between thephotospheric/optical and circumstellar/infrared classification arediscussed.
| M giants at high galactic latitudes: an old metal-rich population?
Spectroscopic and photometric observations are presented for a sample of227 late-M giants in the extended solar neighbourhood, catalogued byStephenson using objective prism plates. The kinematics and scaleheightof these stars suggest that they belong to a mixed population, extendingfrom the old thin disc to the thick disc. They show evidence of thedifferential galactic rotation predicted theoretically. Metallicitieshave been determined from a comparison of TiO band strengths andinfrared colours with model atmospheres for late-type stars, and suggesta mean metallicity close to solar.
| IRAS catalogues and atlases - Atlas of low-resolution spectra
Plots of all 5425 spectra in the IRAS catalogue of low-resolutionspectra are presented. The catalogue contains the average spectra ofmost IRAS poiont sources with 12 micron flux densities above 10 Jy.
| Late M stars found in a hemispheric survey
An objective-prism survey of somewhat more than half the sky, being theportion more than 10 deg from the Galactic plane and north ofdeclination -25 deg, has been completed, using the visual-red spectralregion. From this survey 583 late M stars (mostly type M6 or later) notcontained in the third edition of the variable star catalog or itssupplements are listed. Many identifications with the Caltech Two-MicronSurvey are given. The great majority of the stars are likely to begiants. For an assumed visual absolute magnituge of -0.9, the distanceof the stars from the Galactic plane is well represented by anexponential (barometric) distribution with scale height 1800 pc; or 900pc for an assumed absolute magnitude of zero. The sample may well berelated, therefore, to the recently discussed 'thick disk' component ofgalactic structure. Carbon stars appear to be at least twice asnumerous, relative to late M stars, at large Galactic Z as at small Z.Although difficult to quantify, it appears unlikely that large numbersof these late M stars are undiscovered variables of appreciableamplitude.
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Dades d'Observació i Astrometria
| Constel·lació: | Ursa Major |
| Ascensió Recta: | 11h28m45.06s |
| Declinació: | +49°33'32.5" |
| Magnitud Aparent: | 9.661 |
| Moviment propi RA: | -11.2 |
| Moviment propi Dec: | -7.1 |
| B-T magnitude: | 11.155 |
| V-T magnitude: | 9.785 |
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