Angular diameters of stars from the Mark III optical interferometer., MOZURKEWICH D.; ARMSTRONG J.T.; HINDSLEY R.B.; QUIRRENBACH A.; HUMMEL C.A.; HUTTER D.J.; JOHNSTON K.J.; HAJIAN A.R.; ELIAS II N.M.; BUSCHER D.F.; SIMON R.S., Astron. J., 126, 2502-2520 (2003)
Based upon the values for temperature and radius in combination with the Stefan–Boltzmann law.
Oxygen abundances in halo giants. V. Giants in the fairly metal-rich globular cluster M 71., SNEDEN C.; KRAFT R.P.; LANGER G.E.; PROSSER C.F.; SHETRONE M.D, Astron. J., 107, 1773-1785 (1994)
ดาวดวงแก, arcturus, ในกล, มดาวคนเล, ยงส, ตว, อม, ลส, งเกตการณ, ดเร, มย, j2000, j2000กล, มดาว, กล, มดาวคนเล, ยงส, ตว, ไรต, แอสเซนช, 7sเดคล, เนช, ความส, องสว, างปรากฏ, 04ค, ณสมบ, ชน, ดสเปกตร, มk1, 5iiife, 5ด, ชน, 27ด, ชน, 23ด, ชน, 65ชน, ดดาวแปรแสงดาวแปรแสงnote, . dawdwngaekw dawdwngaekw Arcturus inklumdawkhneliyngstwkhxmulsngektkarncuderimyukh J2000 wisuwt J2000klumdaw klumdawkhneliyngstwirtaexsesnchn 14h 15 m 39 7sedkhlienchn 19 10 56 khwamsxngswangprakt V 0 04khunsmbtichnidsepktrmK1 5IIIFe 0 5dchnisi U B1 27dchnisi B V1 23dchnisi R I0 65chniddawaepraesngdawaepraesngnote category variability H and K emission vary matrdarasastrkhwamerwaenwelng Rv 5 km skarekhluxnthiechphaa m RA 1093 45 mas yr Dec 1999 40 mas yrpharlaelks p 88 98 0 68 masrayathang36 7 0 3 ly 11 24 0 09 pc khwamsxngswangsmburn MV 0 29raylaexiydmwl3 5 1 M rsmi25 7 0 3 2 R khwamsxngswang210 10 3 L xunhphumi4 300 4 Kkhakhwamepnolha20 50 dwngxathitykhwamerwinkarhmuntw v sin i lt 17 km sxayu gt 4 6 109 pichuxxunAlramech Abramech a Bootis 16 Bootes HD 124897 HR 5340 BD 19 2777 GCTP 3242 00 GJ 541 LHS 48 and HIP 69673thankhxmulxangxingxunSIMBADdatadawdwngaekw hrux aexlfakhneliyngstw a Boo a Bootis Alpha Bootis khuxdawvksswangthisudinklumdawkhneliyngstw mikhakhwamsxngswangpraktethakb 0 05 thuxepndawswangthisudladbthi 3 bnthxngfayamratri rxngcakdawsirixusaeladawkhaonpus aetemuxepriybethiybkbdawkhuaexlfakhnkhrungmaxaccaducangaesngkwa ephraadawkhuaexlfakhnkhrungmathng 2 dwngxyuiklknmakcndudwytaeplaesmuxnepndawdwngediywkn dngnndawdwngaekwxacthuxepndawvksswangladbthi 4 bnthxngfakid dawdwngaekwyngxyuinemkhrahwangdawthxngthindwykarkhnhadawdwngaekwxyangngay khuxlakesncakaenwkhnithtrngxxkip haklaktrngxxkipxikkcaecxdawsipka aexlfahyingsaw xangxing aekikh http www stellar database com Scripts search star exe Name Arcturus Angular diameters of stars from the Mark III optical interferometer MOZURKEWICH D ARMSTRONG J T HINDSLEY R B QUIRRENBACH A HUMMEL C A HUTTER D J JOHNSTON K J HAJIAN A R ELIAS II N M BUSCHER D F SIMON R S Astron J 126 2502 2520 2003 Based upon the values for temperature and radius in combination with the Stefan Boltzmann law Oxygen abundances in halo giants V Giants in the fairly metal rich globular cluster M 71 SNEDEN C KRAFT R P LANGER G E PROSSER C F SHETRONE M D Astron J 107 1773 1785 1994 bthkhwamekiywkbdarasastrhruxckrwalwithyaniyngepnokhrng khunsamarthchwywikiphiediyidodyephimkhxmul duephimthi sthaniyxy darasastrekhathungcak https th wikipedia org w index php title dawdwngaekw amp oldid 6893577, wikipedia, วิกิ หนังสือ, หนังสือ, ห้องสมุด,
