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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
| A Study of the Variability of Water Maser Emission in a Sample of Young Stellar Objects
We present results of water maser observations in a sample of youngstellar objects. The observations were made using the Haystack 37 mantenna during a span of time of about eight months. The sample wasselected to study the variability of the water maser emission in youngsources with far-infrared luminosities between 260 and 2.5×10^4L[sun]. The results are shown in a series of plots that allow theanalysis of the variation of the maser emission and to discuss theglobal properties of the sample. The results show that in all theobserved sources the water maser emission varies with time. Based on theobserved variability, the sample shows two kinds of behavior. About halfof the sources show large variations in the peak flux density of atleast one feature (by more than an order of magnitude) in time spansbetween one and several months, while in all the sources there is morethan one feature where the changes in peak flux density are smaller (byless than a factor of 10) but in similar time scales. Finally, thevariability of the observed water maser emission does not show a clearperiodicity pattern in time and we do not find a clear relationshipbetween the luminosity of the sources and the water maser variability.>From a statistical point of view, the H[2]O maser variability can bedescribed as due to small (10%) Gaussian fluctuations in the lineopacity.
| 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.
| 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.
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Наблюдательные данные и астрометрия
| Созвездие: | Печь |
| Прямое восхождение: | 03h43m10.03s |
| Склонение: | -31°01'09.4" |
| Видимая звёздная величина: | 7.185 |
| Расстояние: | 311.526 парсек |
| Собственное движение RA: | 17.2 |
| Собственное движение Dec: | -1.1 |
| B-T magnitude: | 8.998 |
| V-T magnitude: | 7.335 |
Каталоги и обозначения:
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