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The Edinburgh-Cape Blue Object Survey – V. The end: Partial Zones 4–6; Galactic latitudes −50° > b > −90°
Author(s) -
D. Kilkenny,
Hannah L. Worters,
D. O’Donoghue,
C. Koen,
Thea Koen,
N. C. Hambly,
H. T. MacGillivray,
R. S. Stobie
Publication year - 2016
Publication title -
monthly notices of the royal astronomical society
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 2.058
H-Index - 383
eISSN - 1365-8711
pISSN - 0035-8711
DOI - 10.1093/mnras/stw916
Subject(s) - physics , astrophysics , galactic plane , photometry (optics) , stars , metallicity , white dwarf , astronomy , galaxy
Results for the remaining zones of the Edinburgh-Cape (EC) Blue Object survey are presented. These are incomplete, but lie in that part of the South Galactic Cap between 50◦ and 90◦ from the Galactic plane and south of about −12. ◦3 of declination. This part of the survey comprises 79 UK Schmidt Telescope fields covering about 2150 deg2, in which we find 536 blue objects – including hot subdwarfs (∼33 per cent), white dwarfs (∼30 per cent), binaries (∼12 per cent), cataclysmic variables (∼1.5 per cent) and some ‘star-like’ galaxies (∼12 per cent). A further 254 stars observed in the survey, mainly low-metallicity Fand G-type stars, are also listed. Low-dispersion spectroscopic classification is given for all the hot objects and UBV photometry for most of them. Either spectroscopy or photometry is listed for the cooler types.

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