Counts and Colours of Faint Stars in 5 Fields Near the North Galactic Pole

dc.creatorInfante, L.
dc.date1994-08-19
dc.date.accessioned2026-07-07T02:19:22Z
dc.date.available2026-07-07T02:19:22Z
dc.descriptionFaint star number counts in the photographic \jmag band and \bvcol colour distributions are presented for a 1.08 deg$^2$ field near the North Galactic Pole. Due to the excellent star/galaxy discrimination we count stars as faint as \jmag = 23. We compare the number counts and colour distributions in 5 adjacent fields near SA57. The number counts and colour distributions are in very good agreement with previous data. However, we find that the large field-to-field scatter in the colour distributions, which we argue is real, might prevent us setting strong limits on Galactic structure. A simple two component standard model, Bahcall and Soneira (1984), fits the number counts reasonably well at the bright \jmag $< 21$, but fails notably at the faint end, even if a third component is added, as in Reid and Majewski (1993). The standard models are in good agreement with both the number counts and colour distribution at $20 < $\vmag$< 21$. Although the standard models bimodal shape of the colour distribution compares well with the data at $21 < $\vmag$< 21.5$, the number counts of stars are underestimated.
dc.descriptioncompressed uuencoded postscript file, 8 pages, accepted A&A, STARS/1/94
dc.identifierhttps://arxiv.org/abs/astro-ph/9408073
dc.identifierhttp://arxiv.org/abs/astro-ph/9408073
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/9839
dc.subjectAstrophysics
dc.titleCounts and Colours of Faint Stars in 5 Fields Near the North Galactic Pole
dc.typetext

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