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Monthly Notices of the Royal Astronomical Society | 2011

Chemically tagging the Hyades stream: does it partly originate from the Hyades cluster?

L. Pompéia; T. Masseron; Benoit Famaey; S. Van Eck; Ann Jorissen; Ivan Minchev; Arnaud Siebert; Christopher Sneden; Jrd Lépine; Christos Siopis; Gianfranco Gentile; Tyl Dermine; Ester Pasquato; H. Van Winckel; C. Waelkens; Gert Raskin; S. Prins; Wim Pessemier; H. Hensberge; Y. Frémat; L. Dumortier; Olivier Bienayme

The Hyades stream has long been thought to be a dispersed vestige of the Hyades cluster. However, recent analyses of the parallax distribution, of the mass function, and of the actionspace distribution of stream stars have shown it to be rather composed of orbits trapped at a resonance of a density disturbance. This resonant scenario should leave a clearly different signature in the element abundances of stream stars than the dispersed cluster scenario, since the Hyades cluster is chemically homogeneous. Here, we study the metallicity as well as the element abundances of Li, Na, Mg, Fe, Zr, Ba, La, Ce, Nd and Eu for a random sample of stars belonging to the Hyades stream, and compare them with those of stars from the Hyades cluster. From this analysis: (i) we independently confirm that the Hyades stream cannot be solely composed of stars originating in the Hyades cluster; (ii) we show that some stars (namely 2/21) from the Hyades stream nevertheless have abundances compatible with an origin in the cluster; (iii) we emphasize that the use of Li as a chemical tag of the cluster origin of mainsequence stars is very efficient in the range 5500 K ≤ T eff ≤ 6200 K, since the Li sequence in the Hyades cluster is very tight, while at the same time spanning a large abundance range; (iv) we show that, while this evaporated population has a metallicity excess of ∼0.2 dex with respect to the local thin-disc population, identical to that of the Hyades cluster, the remainder of the Hyades stream population has still a metallicity excess of ∼0.06–0.15 dex, consistent with an origin in the inner Galaxy and (v) we show that the Hyades stream can be interpreted as an inner 4:1 resonance of the spiral pattern: this then also reproduces an orbital family compatible with the Sirius stream, and places the origin of the Hyades stream up to 1 kpc inwards from the solar radius, which might explain the observed metallicity excess of the stream population.


Archive | 2016

Editoriaal: Criminele-organisatie-criminaliteit

Antoinette Verhage; Ann Jorissen; Ruth Prins; Jelle Jaspers


Criminele organisaties en organisatiecriminaliteit | 2016

Criminele-organisatie-criminaliteit

Antoinette Verhage; Ann Jorissen; Ruth Prins; Jelle Jaspers


Cahiers Politiestudies | 2016

Criminele organisaties en organisatiecriminaliteit

Antoinette Verhage; Ann Jorissen; Ruth Prins; Jelle Jaspers


Nederland na de crisis / Witteloostuijn, van, A. [edit.] | 2010

Risicomanagment en transparantie rond ondernemingsrisico's

Ann Jorissen; Christoph van der Elst


Nederland na de crisis - Preadviezen van de Koninklijke Vereniging voor Staathuishoudkunde | 2010

Risicomanagement en transparantie rond ondernemingsrisico’s

C.F. van der Elst; Ann Jorissen; A. van Witteloostuijn


Archive | 2009

International Accounting Standards

Ann Jorissen; Nadine Lybaert; Carl Rombaut; Heidi Vander Bauwhede; Ann Verstraeten


Een succesvolle onderneming | 2002

Stramien van een bedrijfsbiografie

Ann Jorissen; Ignace De Beelde


Een succesvolle onderneming | 2002

Boekhouding en jaarrekening van de onderneming

Ignace de Beelde; Ann Jorissen

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C. Waelkens

Katholieke Universiteit Leuven

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Christos Siopis

Université libre de Bruxelles

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Ester Pasquato

Université libre de Bruxelles

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Gert Raskin

Katholieke Universiteit Leuven

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H. Hensberge

Royal Observatory of Belgium

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H. Van Winckel

Katholieke Universiteit Leuven

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L. Dumortier

Royal Observatory of Belgium

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