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ASTRONOMY & ASTROPHYSICS, ISSN 1432-0746, 06/2019, Volume 626, p. A107
Context. Vega and Fomalhaut display a thermal emission brightness that could possibly arise from hot dust near the stars, an inner extension of their planetary... 
ACCELERATION | stars: magnetic field | acceleration of particles | ASTRONOMY & ASTROPHYSICS | MASS | DYNAMICS | GAS | INTERPLANETARY | methods: numerical | interplanetary medium | solar wind | VDP | Astrofysikk, astronomi: 438 | Astrophysics, astronomy: 438 | Physics: 430 | Fysikk: 430 | Mathematics and natural science: 400 | Matematikk og Naturvitenskap: 400
Journal Article
Journal Article
Astronomy and astrophysics (Berlin), ISSN 1432-0746, 2011, Volume 530, p. A21
Journal Article
Journal Article
ISSN 0004-637X, 2011
We have studied the behavior of Fe ions in the slow solar wind, using a fluid model extending from the chromosphere to 1 AU. Emphasis is on elemental "pileup"... 
VDP | Astrofysikk, astronomi: 438 | Astrophysics, astronomy: 438 | Physics: 430 | Fysikk: 430 | Mathematics and natural science: 400 | Matematikk og Naturvitenskap: 400
Journal Article
Journal Article
Astrophysics and space science, ISSN 1572-946X, 2013, Volume 347, Issue 2, pp. 399 - 404
Journal Article