C and N Abundances in Stars at the Base of the Red Giant Branch in M15 (original) (raw)

C and N Abundances in Stars At the Base of the Red Giant Branch in M5

Peter Stetson

2005

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Monthly Notices of the Royal Astronomical Society, 2010

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A spectroscopic study of RGB stars in the globular cluster NGC 2808 with FLAMES

Carla Cacciari

2004

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Helium in first and second-generation stars in globular clusters from spectroscopy of red giants

Valentina D'Orazi

Astronomy and Astrophysics, 2010

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Carbon and Nitrogen Abundances in Stars at the Base of the Red Giant Branch in M5

Peter Stetson

The Astronomical Journal, 2002

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CNONa and 12 C/ 13 C in giant stars of 10 open clusters

Pierre North

Astronomy and Astrophysics, 2009

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Red clump stars of the Milky Way – laboratories of extra-mixing

Ilya Ilyin

Monthly Notices of the Royal Astronomical Society, 2013

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Abundances for a Large Sample of Red Giants in NGC 1851: Hints for a Merger of Two Clusters?

E. Pérez-Careta

The Astrophysical Journal, 2010

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The Astrophysical Journal, 2011

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Gabriele Cescutti

Astronomy & Astrophysics, 2014

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Highly He-rich Matter Dredged Up by Extra Mixing through Stellar Encounters in Globular Clusters

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The Astrophysical …, 2007

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Oxygen and Sodium Abundances in M13 (NGC 6205) Giants: Linking Globular Cluster Formation Scenarios, Deep Mixing, and Post-RGB Evolution

Catherine Pilachowski

The Astrophysical Journal, 2012

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Canonical Extra Mixing in Low‐Mass Red Giants

Pavel Denissenkov

The Astrophysical Journal, 2003

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Low-resolution spectroscopy of main sequence stars belonging to 12 Galactic globular clusters. I. CH and CN band strength variations

Ricardo Carrera

Astronomy & Astrophysics, 2010

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Spectroscopic and photometric evidence of two stellar populations in the Galactic globular cluster NGC 6121 (M 4)

Yazan Momany

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Chemical abundances in bright giants of the globular cluster M62 (NGC 6266)

Alan Alves Brito

Monthly Notices of the Royal Astronomical Society, 2014

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CNONa and 12C/13C in giants of 10 open clusters

Pierre North

2008

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Mass motions and chromospheres of RGB stars in the globular cluster NGC 2808

Yazan Momany

Astronomy and Astrophysics, 2004

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The puzzling MgAl anticorrelation in globular-cluster red giants: primordial plus deep mixing scenario?

Pavel Denissenkov

Arxiv preprint astro-ph/ …, 1997

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Light-element Abundance Variations at Low Metallicity: The Globular Cluster NGC 5466

Rachel Wilkerson

Astronomical Journal, 2010

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DEEP MIXING IN EVOLVED STARS. II. INTERPRETING Li ABUNDANCES IN RED GIANT BRANCH AND ASYMPTOTIC GIANT BRANCH STARS

S. Cristallo, S. Uttenthaler

The Astrophysical Journal, 2011

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TheGaia-ESO Survey: impact of extra mixing on C and N abundances of giant stars

F. Jiménez-Esteban

Astronomy & Astrophysics, 2018

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Dust, pulsation, chromospheres and their rôle in driving mass loss from red giants in Galactic globular clusters

Jacco Van Loon

Astronomy and Astrophysics, 2007

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First stars VI-Abundances of C, N, O, Li, and mixing in extremely metal-poor giants. Galactic evolution of the light elements

Paolo Molaro

Arxiv preprint astro-ph/ …, 2004

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First stars IX - Mixing in extremely metal-poor giants. Variation of the $ \mathsf{^{12}C/^{13}C } $, [Na/Mg] and [Al/Mg] ratios

Paolo Molaro

Astronomy & Astrophysics, 2006

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The extreme chemistry of multiple stellar populations in the metal-poor globular cluster NGC 4833

F. Leone, A. Sollima

Astronomy & Astrophysics, 2014

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Chemical Abundances of Red Giant Stars in the Globular Cluster M107 (NGC 6171)

Catherine Pilachowski

Publ Astron Soc Pac, 2011

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First stars IX - Mixing in extremely metal-poor giants. Variation of the 12 C/ 13 C , [Na/Mg] and [Al/Mg] ratios

Eric Depagne

Astronomy and Astrophysics, 2006

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7 Discovery of Extended Blue Horizontal Branches in Two Metal-Rich Globular Clusters 1

Ben Dorman

2016

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Carbon Abundances of Faint Stars in M13: Evidence of Two Abundance-altering Mechanisms

Peter Stetson

The Astrophysical Journal, 2002

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Discovery of Extended Blue Horizontal Branches in Two Metal-rich Globular Clusters

Ben Dorman

The Astrophysical Journal, 1997

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