VENN , K.a.

Last name: VENN

First name: K.a.

2008 (v1)

Journal article

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Chemical Signatures in Dwarf Galaxies

Venn, K.A. Hill, V.

International audience

Uploaded on: December 3, 2022
2012 (v1)

Journal article

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VLT/FLAMES spectroscopy of red giant branch stars in the Carina dwarf spheroidal galaxy

Lemasle, B. Hill, V. Tolstoy, E.

International audience

Uploaded on: December 3, 2022
2009 (v1)

Journal article

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The dynamical and chemical evolution of dwarf spheroidal galaxies

Revaz, Y. Jablonka, P. Sawala, T.

Astronomy and Astrophysics, 501, pp. 189-206 (2009)

Uploaded on: December 3, 2022
2012 (v1)

Journal article

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Manganese in dwarf spheroidal galaxies

North, P. Cescutti, G. Jablonka, P.

International audience

Uploaded on: December 4, 2022
2010 (v1)

Journal article

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Extremely metal-poor stars in classical dwarf spheroidal galaxies: Fornax, Sculptor, and Sextans

Tafelmeyer, M. Jablonka, P. Hill, V.

International audience

Uploaded on: December 3, 2022
2010 (v1)

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A high-resolution VLT/FLAMES study of individual stars in the centre of the Fornax dwarf spheroidal galaxy

Letarte, B. Hill, V. Tolstoy, E.

International audience

Uploaded on: December 4, 2022
2011 (v1)

Journal article

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Extremely metal-poor stars in classical dwarf spheroidal galaxies: Fornax, Sculptor, and Sextans

Tafelmeyer, M. Jablonka, P. Hill, V.

International audience

Uploaded on: February 22, 2023
2011 (v1)

Journal article

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Extremely metal-poor stars in classical dwarf spheroidal galaxies: Fornax, Sculptor, and Sextans

Tafelmeyer, M. Jablonka, P. Hill, V.

International audience

Uploaded on: December 3, 2022
December 23, 2024 (v1)

Journal article

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The Pristine survey. XXVI. Chemical abundances of subgiant stars of the extremelymetal-poor stream C-19

Bonifacio, P. Caffau, E. François, P.

The C-19 stellar stream is the most metal-poor stream known to date. While its width and velocity dispersion indicate a dwarf galaxy origin, its metallicity spread and abundance patterns are more similar to those of globular clusters (GCs). If it is indeed of GC origin, its extremely low metallicity ( Fe/H =--3.4, estimated from giant stars)...

Uploaded on: January 13, 2025

VENN , K.a.

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