Distances and metallicities for 17 Local Group galaxies

A. W. McConnachie; M. J. Irwin; A. M. N. Ferguson; R. A. Ibata; G. F. Lewis; N. Tanvir

doi:10.1111/j.1365-2966.2004.08514.x

Distances and metallicities for 17 Local Group galaxies

A. W. McConnachie, M. J. Irwin, A. M. N. Ferguson, R. A. Ibata, G. F. Lewis, N. Tanvir

School of Physics and Astronomy

Research output: Contribution to journal › Article › peer-review

Abstract / Description of output

We have obtained Johnson V and Gunni photometry for a large number of Local Group galaxies using the Isaac Newton Telescope Wide Field Camera (INT WFC). The majority of these galaxies are members of the M31 subgroup and the observations are deep enough to study the top few magnitudes of the red giant branch in each system. We previously measured the location of the tip of the red giant branch (TRGB) for Andromeda I, Andromeda II and M33 to within systematic uncertainties of typically

Original language	English
Pages (from-to)	979-997
Journal	Monthly Notices of the Royal Astronomical Society
Volume	356
Issue number	3
DOIs	https://doi.org/10.1111/j.1365-2966.2004.08514.x
Publication status	Published - 1 Jan 2005

Keywords / Materials (for Non-textual outputs)

galaxies: general
Local Group
galaxies: stellar content

Access to Document

10.1111/j.1365-2966.2004.08514.x

Cite this

@article{77e14e60959946d397b639d19e428af9,

title = "Distances and metallicities for 17 Local Group galaxies",

abstract = "We have obtained Johnson V and Gunni photometry for a large number of Local Group galaxies using the Isaac Newton Telescope Wide Field Camera (INT WFC). The majority of these galaxies are members of the M31 subgroup and the observations are deep enough to study the top few magnitudes of the red giant branch in each system. We previously measured the location of the tip of the red giant branch (TRGB) for Andromeda I, Andromeda II and M33 to within systematic uncertainties of typically ",

keywords = "galaxies: general, Local Group, galaxies: stellar content",

author = "McConnachie, {A. W.} and Irwin, {M. J.} and Ferguson, {A. M. N.} and Ibata, {R. A.} and Lewis, {G. F.} and N. Tanvir",

year = "2005",

month = jan,

day = "1",

doi = "10.1111/j.1365-2966.2004.08514.x",

language = "English",

volume = "356",

pages = "979--997",

journal = "Monthly Notices of the Royal Astronomical Society",

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publisher = "Oxford University Press",

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TY - JOUR

T1 - Distances and metallicities for 17 Local Group galaxies

AU - McConnachie, A. W.

AU - Irwin, M. J.

AU - Ferguson, A. M. N.

AU - Ibata, R. A.

AU - Lewis, G. F.

AU - Tanvir, N.

PY - 2005/1/1

Y1 - 2005/1/1

N2 - We have obtained Johnson V and Gunni photometry for a large number of Local Group galaxies using the Isaac Newton Telescope Wide Field Camera (INT WFC). The majority of these galaxies are members of the M31 subgroup and the observations are deep enough to study the top few magnitudes of the red giant branch in each system. We previously measured the location of the tip of the red giant branch (TRGB) for Andromeda I, Andromeda II and M33 to within systematic uncertainties of typically

AB - We have obtained Johnson V and Gunni photometry for a large number of Local Group galaxies using the Isaac Newton Telescope Wide Field Camera (INT WFC). The majority of these galaxies are members of the M31 subgroup and the observations are deep enough to study the top few magnitudes of the red giant branch in each system. We previously measured the location of the tip of the red giant branch (TRGB) for Andromeda I, Andromeda II and M33 to within systematic uncertainties of typically

KW - galaxies: general

KW - Local Group

KW - galaxies: stellar content

U2 - 10.1111/j.1365-2966.2004.08514.x

DO - 10.1111/j.1365-2966.2004.08514.x

M3 - Article

SN - 0035-8711

VL - 356

SP - 979

EP - 997

JO - Monthly Notices of the Royal Astronomical Society

JF - Monthly Notices of the Royal Astronomical Society

IS - 3

ER -

Distances and metallicities for 17 Local Group galaxies

Abstract / Description of output

Keywords / Materials (for Non-textual outputs)

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