Inici     Començant     Sobreviure a l'Univers    
Inhabited Sky
    News@Sky     Astro Fotografia     La Col·lecció     Fòrum     Blog New!     FAQ     Premsa     Login  

HD 56664


Contingut

Imatges

Carregar la teva Imatge

DSS Images   Other Images


Articles Relacionats

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.

Photometry of Suspected UU Her-Stars
Not Available

The UU Her-type stars - Possible tracers of recent star formation at high galactic latitudes
A general review of the group of UU Her-type stars proposed recently asa possible new type of variables is given. The available observations(spectra and photometry) reveal them as luminous Population I F-typesupergiants of normal composition. This fact contradicts their greatdistances above the galactic plane. As there is no reason so far todistrust the results from the spectroscopic analyses and photometry, thegalactic plane should be excluded as a possible birthplace of the UUHer-stars. In this respect they might probably indicate that recent starformation (though occasional) from already enriched material waspossible at high galactic latitudes. Moreover, normal Main-SequenceB-stars seem now also to be found there. Much attention is paid to thespecific semiregular variability of the UU Her-stars. The type ofpulsations remains conjectural, but simple radial pulsations shouldobviously be ruled out.

Enviar un nou article


Enllaços Relacionats

  • - No s'ha trobat enllaços -
Enviar un nou enllaç


Membre dels grups següents:


Dades d'Observació i Astrometria

Constel·lació:Camelopardalis
Ascensió Recta:07h21m47.64s
Declinació:+60°55'40.6"
Magnitud Aparent:8.433
Distancia:200.401 parsecs
Moviment propi RA:-10.6
Moviment propi Dec:-29.3
B-T magnitude:8.772
V-T magnitude:8.461

Catàlegs i designacions:
Noms Propis   (Edit)
HD 1989HD 56664
TYCHO-2 2000TYC 4111-14-1
USNO-A2.0USNO-A2 1500-04823163
HIPHIP 35685

→ Sol·licitar més catàlegs i designacions de VizieR