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Effective temperature scale and bolometric corrections from 2MASS photometry
We present a method to determine effective temperatures, angularsemi-diameters and bolometric corrections for population I and II FGKtype stars based on V and 2MASS IR photometry. Accurate calibration isaccomplished by using a sample of solar analogues, whose averagetemperature is assumed to be equal to the solar effective temperature of5777 K. By taking into account all possible sources of error we estimateassociated uncertainties to better than 1% in effective temperature andin the range 1.0-2.5% in angular semi-diameter for unreddened stars.Comparison of our new temperatures with other determinations extractedfrom the literature indicates, in general, remarkably good agreement.These results suggest that the effective temperaure scale of FGK starsis currently established with an accuracy better than 0.5%-1%. Theapplication of the method to a sample of 10 999 dwarfs in the Hipparcoscatalogue allows us to define temperature and bolometric correction (Kband) calibrations as a function of (V-K), [m/H] and log g. Bolometriccorrections in the V and K bands as a function of T_eff, [m/H] and log gare also given. We provide effective temperatures, angularsemi-diameters, radii and bolometric corrections in the V and K bandsfor the 10 999 FGK stars in our sample with the correspondinguncertainties.
| Radial velocities. Measurements of 2800 B2-F5 stars for HIPPARCOS
Radial velocities have been determined for a sample of 2930 B2-F5 stars,95% observed by the Hipparcos satellite in the north hemisphere and 80%without reliable radial velocity up to now. Observations were obtainedat the Observatoire de Haute Provence with a dispersion of 80Ä,mm(-1) with the aim of studying stellar and galactic dynamics.Radial velocities have been measured by correlation with templates ofthe same spectral class. The mean obtained precision is 3.0 km s(-1)with three observations. A new MK spectral classification is estimatedfor all stars. Based on observations made at the Haute ProvenceObservatory, France and on data from The Hipparcos Catalogue, ESA.Tables 4, 5 and 6 are only available in electronic form at the CDS viaanonymous ftp to cdsarc.u-strasbg.fr or viahttp://cdsweb.u-strasbg.fr/Abstract.htm
| ANS UV observations of external galaxies. II - UV photometry of M 31, M 33, M 81, M 101, NGC 2403 and several Zwicky galaxies
Five-color area-integrated UV photometric results are given of 2.5 x 2.5arcmin fields in the galaxies M 31, M 33, M 81, M 101 and NGC 2403. Mostof these fields are centered on bright HII regions. The UV fluxesdetected are generally representative of OB associations. The data forthe nearby galaxies indicate radial gradients in brightness and colorwithin these galaxies. In addition, results are presented of a survey ofZwicky-type dwarf galaxies.
| V-V 144, an Exploding Galaxy?.
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| Takýmyýldýz: | Buyuk Ayi |
| Sað Açýklýk: | 11h25m35.00s |
| Yükselim: | +54°24'30.7" |
| Görünürdeki Parlaklýk: | 8.548 |
| Uzaklýk: | 257.069 parsek |
| özdevim Sað Açýklýk: | -22.3 |
| özdevim Yükselim: | -11.3 |
| B-T magnitude: | 8.806 |
| V-T magnitude: | 8.57 |
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