Virtual Journal of Nuclear Astrophysics
Edited by
Sudhanva Lalit
, Michigan State University and
Pelagia Tsintari
, Michigan State University
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Results 1 - 4 of 4
A Plasmoid Model for Mass Loss from Stars on the Upper Red Giant Branch: The Mass-loss Rate is Controlled by the Number of Density Scale Heights in the Convection Zone
Virtual Journal - Volume 23, Issue 26 - article #80
J. MacDonald
,
D. J. Mullan
The Astrophysical Journal Letters
https://doi.org/10.3847/2041-8213/adf6ae
Magneto-convective models of red dwarfs: constraints imposed by the lithium abundance
Virtual Journal - Volume 13, Issue 3 - article #6
J. MacDonald
,
D. J. Mullan
arXiv.org - Astrophysics - Volume: 2015, Issue: 23 Jan
arXiv:1501.04550
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Why is the Sun so large?
Virtual Journal - Volume 3, Issue 50 - article #1
D. J. Mullan
American Journal of Physics – Vol. 74, Issue 1 – December 2005
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Onset of Mass Loss in Red Giants: Association with an Evolutionary Event
Virtual Journal - Volume 1, Issue 1 - article #26
D. J. Mullan
and
J. MacDonald
The Astrophysical Journal, Volume 591, Number 2, Part 1
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