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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 Henize sample of S stars. I. The technetium dichotomy
This paper is the first one in a series investigating the properties ofthe S stars belonging to the Henize sample (205 S stars with delta<-25(deg) and R<10.5) in order to derive the respective properties(like galactic distribution and relative frequencies) of intrinsic (i.e.genuine asymptotic giant branch) S stars and extrinsic (i.e. postmass-transfer binary) S stars. High-resolution (R=30 000 to 60 000)spectra covering the range lambda lambda4230 -4270 Angstroms have beenobtained for 76 S stars, 8 M stars and 2 symbiotic stars. The lambda4262Angstroms and lambda4238 Angstroms blends involving a Tc I line wereanalysed separately and yield consistent conclusions regarding thepresence or absence of technetium. Only one `transition' case (Hen 140 =HD 120179, a star where only weak lines of technetium are detectable) isfound in our sample. A resolution greater than R =30 000 is clearlyrequired in order to derive unambiguous conclusions concerning thepresence or absence of technetium. The Tc/no Tc dichotomy will becorrelated with radial velocity and photometric data in a forthcomingpaper. Based on observations carried out at the European SouthernObservatory (ESO, La Silla, Chile)
| The 74th Special Name-list of Variable Stars
We present the Name-list introducing GCVS names for 3153 variable starsdiscovered by the Hipparcos mission.
| Vitesses radiales. Catalogue WEB: Wilson Evans Batten. Subtittle: Radial velocities: The Wilson-Evans-Batten catalogue.
We give a common version of the two catalogues of Mean Radial Velocitiesby Wilson (1963) and Evans (1978) to which we have added the catalogueof spectroscopic binary systems (Batten et al. 1989). For each star,when possible, we give: 1) an acronym to enter SIMBAD (Set ofIdentifications Measurements and Bibliography for Astronomical Data) ofthe CDS (Centre de Donnees Astronomiques de Strasbourg). 2) the numberHIC of the HIPPARCOS catalogue (Turon 1992). 3) the CCDM number(Catalogue des Composantes des etoiles Doubles et Multiples) byDommanget & Nys (1994). For the cluster stars, a precise study hasbeen done, on the identificator numbers. Numerous remarks point out theproblems we have had to deal with.
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| Takýmyýldýz: | Yay |
| Sað Açýklýk: | 19h22m25.67s |
| Yükselim: | -31°56'11.8" |
| Görünürdeki Parlaklýk: | 6.976 |
| Uzaklýk: | 413.223 parsek |
| özdevim Sað Açýklýk: | -5 |
| özdevim Yükselim: | -9.3 |
| B-T magnitude: | 9.16 |
| V-T magnitude: | 7.157 |
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