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Asymptotic Giant Branch Stars

2000
Hydrostatic nucleosynthesis modifies the internal composition of low and intermediate mass stars(M
Oscar Straniero   +4 more
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Nucleosynthesis in asymptotic giant branch stars

AIP Conference Proceedings, 2014
The nucleosynthesis in asymptotic giant branch stars (briefly: AGB)is a challenging and fascinating subject in the theory of stellar evolution and important for observations as well. This is because about of half the heavy elements beyond iron are synthesized during thermal pulsation phases of these stars.
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Large Telescopes and Asymptotic Giant Branch Stars

AIP Conference Proceedings, 2005
There are many ways in which observations with large telescopes are improving our understanding of evolution on the Asymptotic Giant Branch. Perhaps more importantly AGB stars also offer huge potential to probe the nature of low‐ and intermediate‐mass populations over a very considerable range of distances and in a variety of environments.
Michael Feast, Patricia A. Whitelock
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Asymptotic giant branch stars in the ISOGAL survey

2000
We present and analyse the data of a field at 1 = 0o, b = +1o from the ISOGAL survey of selected areas of the inner Galactic bulge at 15 and 7 ?m. In combination with IJKs data from the near-infrared southern sky survey DENIS, the ISOCAM data allow the first detailed study of infrared stellar populations in very obscured regions of the inner Galaxy ...
Ojha, D. K.   +3 more
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Circumstellar envelopes and Asymptotic Giant Branch stars

The Astronomy and Astrophysics Review, 1996
Red giants are sometimes surrounded by envelopes, the result of the ejection of stellar matter at a large rate ( $\dot M> 10^{-7}M_\odot$ /yr) and at a low velocity (10 km/s). In this review the envelopes are discussed and the relation between stars and envelope: what stars combine with what envelopes?
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