Results 191 to 200 of about 3,760 (219)

Unraveling the complexity of rat object vision requires a full convolutional network and beyond. [PDF]

Patterns (N Y)
Muratore P, Alemi A, Zoccolan D.
europepmc   +1 more source

Atacama Large Aperture Submillimeter Telescope (AtLAST) science: Probing the transient and time-variable sky. [PDF]

Open Res Eur
Orlowski-Scherer J, Maccarone T, Bright J, Kamiński T, Koss M, Mohan A, Miguel Montenegro-Montes F, Næss S, Ricci C, Severgnini P, Stanke T, Vignali C, Wedemeyer S, Booth M, Cicone C, Di Mascolo L, Johnstone D, Mroczkowski T, Cordiner M, Greiner J, Hatziminaoglou E, van Kampen E, Klaassen P, Lee M, Liu D, Saintonge A, Smith M, Thelen A.   +27 more
europepmc   +1 more source

Hydrogen ejection from hydrocarbons: Characterization and relevance in soot formation and interstellar chemistry. [PDF]

Proc Natl Acad Sci U S A
Hendrix J, Hait D, Michelsen HA, Head-Gordon M.   +3 more
europepmc   +1 more source

Asymmetries in asymptotic giant branch stars and their winds

Astronomy & Astrophysics
Wiegert, Joachim, Freytag, Bernd, Höfner, Susanne   +2 more
openaire   +2 more sources

Infrared studies of asymptotic giant branch stars

, 1987
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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.
exaly   +2 more sources

Asymptotic giant branch and super-asymptotic giant branch stars: modelling dust production at solar metallicity [PDF]

Monthly Notices of the Royal Astronomical Society, 2017
We present dust yields for asymptotic giant branch (AGB) and super-asymptotic giant branch (SAGB) stars of solar metallicity. Stars with initial mass 1.5 M⊙ ≤ Mini ≤ 3 M⊙ reach the carbon star stage during the AGB phase and produce mainly solid carbon ...
F Dell'Agli, D A García-Hernández, R Schneider   +2 more
exaly   +2 more sources

Circumstellar envelopes of asymptotic giant branch stars

, 2018
At the end of their lives, stars with masses between 0.8 and 8 solar masses (M⊙) enter an evolutionary phase called asymptotic giant branch (AGB), during which they develop intense stellar winds. AGB stars are important producers of chemical elements, created through stellar nucleosynthesis processes in the stellar interior and particularly in thin ...
Brunner, Magdalena
openaire   +2 more sources

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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Asymptotic Giant Branch Stars

2000
O. Straniero, M. Limongi, A. Chieffi, R. Gallino, M. Busso   +4 more
openaire   +1 more source