... LGS 3 c - m diagram ( Lee 1995 , Mould 1997 ) is similar dominance of apparently old metal - poor red giants . As is the case for Phoenix , the mean abundance for LGS 3 determined from the mean colour of the red giant branch is such that ...
... LGS 3 have been published by Christian and Tully ( 1983 ) 11 ] and by Schild ( 1980 ) 12 ] . The former authors obtained UBV images and de- rived a color - magnitude diagram . They remarked that " LGS 3 is unique in one respect . In all ...
... LGS3 Edouard J. Bernard for the LCID Team † Instituto de Astrofísica de Canarias , E - 38205 La Laguna , Tenerife , Spain email : ebernard@iac.es Abstract . We present preliminary results concerning the search for short - period ...
... LGS3, 257. 27. Santayana, LGS3, 260. Santayana eventually did not, in fact, take a box of books with him, only some copies of his own books and manuscripts. This tug between Spain and Italy, is clarified to some extent by Graziella ...
... lgs. 3 lgs. 3 lgs. 3 lgs. 1 property Cavineña East Kewa Murui Huitoto Eastern Khanty Bardi Burushaski Thompson 2 properties – – – Semai Tohono O'odham 3 or more properties – Lao Pacoh Koho – The specific phonological differences between ...
... LGS - 3 MUL MERIDIAN LGS - 3 MUL 4398 4598 7151 7551 8276 13783 8676 14583 53068 56068 MISSISSIPP ! POWER CO / 10,40 MISSISSIPPI POWER CO / 11,40 80600 MISSISSIPPI POWER ( 3/10 85600 MISSISSIPPI POWER 03/11 MISSISSIPPI POWER & LIGHT CO ...
... ( LGS , 3 : 278 ) ; 1 August 1926 to Otto Kyllmann ( LGS , 3 : 285 ) ; 11 August 1926 to Charles Augustus Strong ( LGS , 3 : 287 ) . 541 August 1926 to Otto Kyllmann ( LGS , 3 : 285 ) ; 16 May 1926 to Charles Augustus Strong ( LGS , 3 ...
... Lgs . 3 To ; A. C. 6 ins . B 480 ; S. T40 ; L. 10 ; 12. Grey Wagtail . ( M. cinerea ) . About the same as the last . 13. Wheat - ear . ( S. œnanthe ) . B. 282 ; S. ‡ ‡ ; L. 10 ; Lgs . 5 ; A. C. 9 ins . & ; H. 4 14. Swallow . ( H ...
... LGS - 3 respectively . Among this sample of galaxies , LGS - 3 is the only one to have a symmetrical , centrally peaked HI distribution . In all the other dwarfs , the HI distribution is more clumpy , with HI loops , arcs , and multiple ...