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https://doi.org/10.1023/a:1017518411367

A New Photometric Look at M51

Mar 1, 2001
Astrophysics and Space Science
V Vansevičius

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A New Photometric Look at M51

ReferencesShowing 8 of 19 papers

1545
10.1086/172385

Spectral evolution of stellar populations using isochrone synthesis

Mar 1, 1993
The Astrophysical Journal
Gustavo Bruzual A + 1 more

115
10.1086/167733

Spiral arm amplitude variations and pattern speeds in the grand design galaxies M51, M81, and M100

Aug 1, 1989
The Astrophysical Journal
Bruce G Elmegreen + 2 more

24
10.1086/176836

The Revised MG 2 Index as a Metallicity Indicator for Stellar Systems: Giant Elliptical Galaxies and Bulges

Feb 1, 1996
The Astrophysical Journal
E Casuso + 3 more

62
10.1038/359129a0

Direct measurement of the optical depth in a spiral galaxy

Sep 10, 1992
Nature
Raymond E White + 1 more

182
10.1086/512787

Planetary Nebulae as Standard Candles. XI. Application to Spiral Galaxies

Apr 10, 1997
The Astrophysical Journal
John J Feldmeier + 2 more

31
10.1007/978-94-011-0381-7

The Opacity of Spiral Disks

Jan 1, 1995
Jonathan I Davies

106
10.1093/mnras/253.2.245

Abundance analysis of giant H II regions in M51

Nov 1, 1991
Monthly Notices of the Royal Astronomical Society
Angeles I Díaz + 4 more

50
10.1086/176999

Tracing the Dynamics of Disk Galaxies with Optical and Infrared Surface Photometry: Color Gradients in M99

Apr 1, 1996
The Astrophysical Journal
Rosa A Gonzalez + 1 more

CitationsShowing 1 of 1 papers

Research Article
74
10.1051/0004-6361:20047024

The radial extinction profiles of late-type galaxies

Aug 23, 2004
Astronomy & Astrophysics
S Boissier + 4 more

We have used UV (FOCA) and FIR (IRAS) images of six nearby late type galaxies to study the radial variation of the UV extinction (deduced from the FIR/UV ratio). We compare the UV extinction gradient with other extinction indicators (Balmer decrement) and search for a relation between the extinction, the metallicity and the gas surface density among our galaxies. We detect in our small sample a clear relation between extinction and metallicity. These observed relations are used to calibrate an empirical recipe useful for extinction correction in the UV, visible and near-infrared images of late type galaxies.