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Cited by 349

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Distance to M31 with the [ITAL]Hubble Space Telescope[/ITAL] and [ITAL]Hipparcos[/ITAL] Red Clump Stars

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Stanek, K. Z., Garnavich, P. M.·1998·The Astrophysical Journal

Abstract

Following the approach by Paczyński & Stanek, we compare the red clump stars with parallaxes known to better than 10% in the Hipparcos catalog with the red clump stars observed in three fields in M31 using the Hubble Space Telescope . There are ~600 and ~6300 such stars in the two data sets, respectively. The local red clump luminosity function is well represented by a Gaussian with the peak at M I,m =-0.23 and the dispersion σ RC ≈ 0.2 mag. This allows a single-step determination of the distance modulus to M31, μ 0, M31 =24.471 ± 0.035 ± 0.045 mag (statistical plus systematic error), and the corresponding distance, R M31 =784 ± 13 ± 17 kpc. The number of red clump stars is large enough that the formal statistical error in the distance is only ≲2%. We also correct the treatment of the local interstellar extinction by Paczyński & Stanek, and we obtain the Galactocentric distance modulus, μ 0, GC =14.57 ± 0.04 ± 0.04 mag (statistical plus systematic error), and the corresponding Galactocentric distance, R 0 =8.2 ± 0.15 ± 0.15 kpc.

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Metadata

Authors
Stanek, K. Z., & Garnavich, P. M.
Venue
The Astrophysical Journal
Published
1998-08-20
Volume
503
Issue
2
Pages
L131-L134
ISSN
0004-637X (ISSN-L)
OpenAlex
W1580006248
Cited by
349
References
14
FWCI
14.28
Type
journal article
Language
en
Open access
bronze

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CoChat. (2026). Citation check: Distance to M31 with the [ITAL]Hubble Space Telescope[/ITAL] and [ITAL]Hipparcos[/ITAL] Red Clump Stars. https://app.cochat.ai/papers/10.1086/311539
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Stanek, K. Z., & Garnavich, P. M. (1998). Distance to M31 with the [ITAL]Hubble Space Telescope[/ITAL] and [ITAL]Hipparcos[/ITAL] Red Clump Stars. The Astrophysical Journal. https://doi.org/10.1086/311539

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