Field #3 of the Palomar-Groningen Survey II. Near-infrared photometry of semiregular variables

Details Field #3 of the Palomar-Groningen Survey II. Near-infrared photometry of semiregular variables Field #3 of the Palomar-Groningen Survey II. Near-infrared photometry of semiregular variables

1998-07-30

arxiv.org/abs/astro-ph/9807321v2

Astronomy and Astrophysics

Astrophysics

14 pages LaTeX (2 tables, 8 figures), to appear in A&A 338 (1998); minor modifications in text

Scientific paper

Near-infrared photometry (JHKL'M) was obtained for 78 semiregular variables (SRVs) in field #3 of the Palomar-Groningen survey (PG3, l=0, b=-10). Together with a sample of Miras in this field a comparison is made with a sample of field SRVs and Miras. The PG3 SRVs form a sequence (period-luminosity & period-colour) with the PG3 Miras, in which the SRVs are the short period extension to the Miras. The field and PG3 Miras follow the same P/(J--K)o relation, while this is not the case for the field and PG3 SRVs. Both the PG3 SRVs and Miras follow the SgrI period-luminosity relation adopted from Glass et al. (1995, MNRAS 273, 383). They are likely pulsating in the fundamental mode and have metallicities spanning the range from intermediate to approximately solar.

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