... A1V 3.778 -0.001 0.029 -0.005 -0.010 ep Aqr "BS1544" 04 50 36.7 08 54 01 !A1Vn 4.355 0.02 -0.03 0.014 0.039 pi Ori -------------------------------------------- There is significant fringing in the order containing the Ca triplet. ...
... Name m2 Cet n Ori g Hya h Crt h Vir 108 Vir 58 Aql v Aqr f Peg 29 Psc HD 15318 30739 74280 100889 114330 129956 188350 198001 214923 224926 V 4.279 4.355 4.295 4.70 4.375 5.681 5.62 3.778 3.40 5.120 NOTE.хUnits of right ascension are hours, minutes, and ...
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Ссылки http://www.mso.anu.edu.au/~bessell/FTP/Oldspectrophotometry/aa_paper_on_spectrophotometry.pdf -- 231.5 Кб -- 29.11.2004 Похожие документы
... This is slightly cooler than t solar metal abundance and may be interpreted as correction for unaccounted non-LTE effects on th keting in the most luminous objects, i.e. Ori an in the present case. ...
RSAA Annual Report 2001 RESEARCH SCHOOL OF ASTRONOMY & ASTROPHYSICS ANNUAL REPORT 2001 The Institute of Advanced Studies The Australian National University 1 RSAA Annual Report 2001 Research School of Astronomy & Astrophysics Institute of Advanced...
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Ссылки http://www.mso.anu.edu.au/annualReport/2001/annrep_2001.pdf -- 398.8 Кб -- 15.10.2004 Похожие документы