Dust production rate of asymptotic giant branch stars in the Magellanic Clouds

We compare theoretical dust yields for stars with masses 1 ≤ m star ≤ 8 M⊙ and metallicities 0.001 ≤ Z ≤ 0.008 with observed dust production rates (DPRs) using carbon-rich and oxygen-rich asymptotic giant branch (C-AGB and O-AGB) stars in the Large and Small Magellanic Clouds (LMC and SMC). The meas...

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Veröffentlicht in:	Monthly notices of the Royal Astronomical Society 2014-08, Vol.442 (2), p.1440-1450
Hauptverfasser:	Schneider, Raffaella, Valiante, Rosa, Ventura, Paolo, dell'Agli, Flavia, Di Criscienzo, Marcella, Hirashita, Hiroyuki, Kemper, Francisca
Format:	Artikel
Sprache:	eng
Schlagworte:	Astronomy Comparative analysis Dust Oxygen Stars & galaxies
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