시작하기     To Survive in the Universe    
Inhabited Sky
    News@Sky     천체사진     컬렉션     포럼     Blog New!     질문및답변     출판     로그인  

HD 56664


내용

사진

사진 업로드

DSS Images   Other Images


관련 글

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.

새 글 등록


관련 링크

  • - 링크가 없습니다. -
새 링크 등록


다음 그룹에 속해있음:


관측 및 측정 데이터

별자리:기린자리
적경:07h21m47.64s
적위:+60°55'40.6"
가시등급:8.433
거리:200.401 파섹
적경상의 고유운동:-10.6
적위상의 고유운동:-29.3
B-T magnitude:8.772
V-T magnitude:8.461

천체목록:
일반명   (Edit)
HD 1989HD 56664
TYCHO-2 2000TYC 4111-14-1
USNO-A2.0USNO-A2 1500-04823163
HIPHIP 35685

→ VizieR에서 더 많은 목록을 가져옵니다.