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Methods used for the quantitative classification of metal-deficient stars in the Vilnius photometric...
One of the main uses of the Hipparcos astrometric parameters is the calibration of stellar luminosit...
We combined the (K (s) , J-K (s) ) data in Laney et al. (Mon. Not. R. Astron. Soc. 419:1637, 2012) w...
We calculate the average absolute magnitude for Hipparcos single K0V stars, using a theoretical curv...
We analyse a sample of about 500 MK standards of cool spectral types (G to M) for to compare the v...
. Hipparcos parallaxes of high-amplitude ffi Scuti stars are used to derive a period-luminosity rel...
The mean absolute magnitude of the Am stars was determined from statistical parallaxes. The material...
The spectroscopic absolute magnitudes and parallaxes of 200 A stars have been determined. The materi...
We compare the absolute visual magnitude of the majority of bright O stars in the sky as predicted f...
We present absolute magnitude estimates for a number of peculiar star groups, defined on the basis o...
International audienceA good knowledge of both accuracy and precision of the Hipparcos parallaxes is...
Context. Determination of absolute parallaxes by means of a scanning astrometric satellite such as H...
Context. Accurate measurements of diameters of trans-Neptunian objects (TNOs) are extremely difficul...
The basic data discussed here consist of parallaxes and apparent magnitudes of more than 6000 stars ...
The position of different kinds of CP stars of the upper Main Sequence (i.e. Am stars and the four c...
Methods used for the quantitative classification of metal-deficient stars in the Vilnius photometric...
One of the main uses of the Hipparcos astrometric parameters is the calibration of stellar luminosit...
We combined the (K (s) , J-K (s) ) data in Laney et al. (Mon. Not. R. Astron. Soc. 419:1637, 2012) w...
We calculate the average absolute magnitude for Hipparcos single K0V stars, using a theoretical curv...
We analyse a sample of about 500 MK standards of cool spectral types (G to M) for to compare the v...
. Hipparcos parallaxes of high-amplitude ffi Scuti stars are used to derive a period-luminosity rel...
The mean absolute magnitude of the Am stars was determined from statistical parallaxes. The material...
The spectroscopic absolute magnitudes and parallaxes of 200 A stars have been determined. The materi...
We compare the absolute visual magnitude of the majority of bright O stars in the sky as predicted f...
We present absolute magnitude estimates for a number of peculiar star groups, defined on the basis o...
International audienceA good knowledge of both accuracy and precision of the Hipparcos parallaxes is...
Context. Determination of absolute parallaxes by means of a scanning astrometric satellite such as H...
Context. Accurate measurements of diameters of trans-Neptunian objects (TNOs) are extremely difficul...
The basic data discussed here consist of parallaxes and apparent magnitudes of more than 6000 stars ...
The position of different kinds of CP stars of the upper Main Sequence (i.e. Am stars and the four c...
Methods used for the quantitative classification of metal-deficient stars in the Vilnius photometric...
One of the main uses of the Hipparcos astrometric parameters is the calibration of stellar luminosit...
We combined the (K (s) , J-K (s) ) data in Laney et al. (Mon. Not. R. Astron. Soc. 419:1637, 2012) w...