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Journal of Astronomy and Space Sciences
Article . 2008 . Peer-reviewed
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Journal of Astronomy and Space Sciences
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Journal of Astronomy and Space Sciences
Article . 2008
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https://dx.doi.org/10.5140/jas...
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The Near-IR TRGB Magnitude and Distance Modulus to NGC 185

descriptionPublicationkeyboard_double_arrow_right Article 15 Sep 2008 English Publisher:The Korean Space Science SocietyJournal:Journal of Astronomy and Space Sciences, volume 25, pages 245-248 (issn: 2093-5587, Copyright policy )
Authors: Y.-J. Sohn; A. Kang; W. Han; J.-H. Park; H.-I. Kim; J.-W. Kim; I.-G. Shin; +1 Authors

doi: 10.5140/jass.2008.25.3.245

The Near-IR TRGB Magnitude and Distance Modulus to NGC 185

Abstract

We determined values of distance modulus to nearby dwarf galaxy NGC 185 from the Tip of Red-Giant Branch (TRGB) method. Apparent magnitudes of the TRGB are estimated from the near-infrared JHK luminosity functions (LFs) of the resolved giant branch stars. Theoretical absolute magnitudes of the TRGB in near-infrared bands have been extracted from the Yonsei-Yale isochrones. The observed apparent and theoretical absolute magnitudes of the TRGB provide values of distance modulus to NGC 185 as (m - M).

Keywords

NGC 185, Astronomy, QB1-991, TRGB, distance modulus, near-infrared

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selected citations
These citations are derived from selected sources.
This is an alternative to the "Influence" indicator, which also reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Citations provided by BIP!
popularity
This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network.
BIP!Popularity provided by BIP!
influence
This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Influence provided by BIP!
impulse
This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network.
BIP!Impulse provided by BIP!
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