Short-Lived Nuclei in the Early Solar System: A Low Mass Stellar Source?

By Maurizio Busso, Roberto Gallino, G. Wasserburg. Publications Astronomical Society of Australia, 2003

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View Paper: https://www.semanticscholar.org/paper/c05c722988f76b79631b5cd92f3daf5389857356

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Citations in the corpus

The Birth Environment of the Solar System (2010, background): “…differs from many previous discussions that primarily focus on the origin of the short-lived radio isotopes (Wadhwa et al. 2007; Goswami & Vanhala 2000; Busso et al. 1999, 2003; Wasserburg et al. 2006) and/or the thermodynamic history of the early solar system (e.g., Krot et al. 2005ab, 2008).”
Astrophysics with Extraterrestrial Materials (2016, background): “F or p er so na l u se o nl y. lifetimes require direct injection into the solar nebula by a stellar source (Wasserburg et al. 2006).”
THE SPITZER c2d LEGACY RESULTS: STAR-FORMATION RATES AND EFFICIENCIES; EVOLUTION AND LIFETIMES (2008, background): “The presence of short-lived nuclei such as 60Fe, 41Ca, 53Mn, and 26Al in planetesimals must, in part, arise from the timely nucleosynthetic input from nearby AGB stars and/or supernovae (Wasserburg et al. 2006).”
26 Al- 26 Mg and 207 Pb- 206 Pb systematics of Allende CAIs: Canonical solar initial 26 Al/ 27 Al ratio reinstated (2008, background): “…limit the possible sources of 41Ca, 26Al and other short-lived radionuclides in the early Solar System (energetic particle irradiation near the proto-Sun (e.g., Shu et al., 1996; Gounelle et al., 2006) vs. injection from nearby stars (e.g., Sahijpal et al., 1998; Wasserburg et al., 2006).”
Aluminum-, Calcium- and Titanium-rich Oxide Stardust in Ordinary Chondrite Meteorites (2008, background): “Significant attention has been paid to the production of 41Ca since this short-lived isotope has been inferred to have been present in the early solar system (Srinivasan et al. 1994; Wasserburg et al. 2006).”
The s-Process in Low Metallicity Stars. II. Interpretation of High-Resolution Spectroscopic Observations with AGB models (2011, background): “…to about 20 (Boothroyd & Sackmann 1988; Busso et al. 1999). dicted to occur in low-mass AGB stars (see Nollett et al. 2003; Domı́nguez et al. 2004; Wasserburg et al. 1995, 2006; Busso et al. 2010), and may decrease 12C in the envelope while 14N increases (Wasserburg et al. 1995);…”
HETEROGENEOUS DISTRIBUTION OF 26Al AT THE BIRTH OF THE SOLAR SYSTEM (2010, background): “…and themanner inwhich it was injected into the solar system remain controversial: it could have been produced by an asymptotic giant branch star (Wasserburg et al. 2006), a type II supernova (e.g., Meyer 2005), or by a wind from a massive star prior to its explosion as a type Ib ⁄ Ic supernova…”