Pulsation-induced atmospheric dynamics in M-type AGB stars

Author： Liljegren S.   Höfner S.   Eriksson K.   Nowotny W.  

Publisher： Edp Sciences

E-ISSN： 1432-0746|606|issue|A6-A6

ISSN： 0004-6361

Source： Astronomy & Astrophysics, Vol.606, Iss.issue, 2017-09, pp. : A6-A6

Disclaimer: Any content in publications that violate the sovereignty, the constitution or regulations of the PRC is not accepted or approved by CNPIEC.

Previous Menu Next

Abstract

Context. Wind-driving in asymptotic giant branch (AGB) stars is commonly attributed to a two-step process. First, matter in the stellar atmosphere is levitated by shock waves, induced by stellar pulsation, and second, this matter is accelerated by radiation pressure on dust, resulting in a wind. In dynamical atmosphere and wind models the effects of the stellar pulsation are often simulated by a simplistic prescription at the inner boundary.

Related content

“Thermal” SiO radio line emission towards M-type AGB stars: A probeof circumstellar dust formation and dynamics

By  

Astronomy & Astrophysics, Vol. 411, Iss. 2, 2003-11 ,pp. : 123-147 (25)

Edp Sciences

Access to resources Recommend Favorite

Winds of M-type AGB stars driven by micron-sized grains

By  

Astronomy & Astrophysics, Vol. 491, Iss. 2, 2008-11 ,pp. : L1-L4 (NaN)

Edp Sciences

Access to resources Recommend Favorite

Water isotopologues in the circumstellar envelopes of M-type AGB stars⋆

By Danilovich T.   Lombaert R.   Decin L.   Karakas A.   Maercker M.   Olofsson H.  

Astronomy & Astrophysics, Vol. 602, Iss. issue, 2017-05 ,pp. : A14-A14 (NaN)

Edp Sciences

Access to resources Recommend Favorite

Sulphur molecules in the circumstellar envelopes of M-type AGB stars⋆

By Danilovich T.   De Beck E.   Black J. H.   Olofsson H.   Justtanont K.  

Astronomy & Astrophysics, Vol. 588, Iss. issue, 2016-03 ,pp. : A119-A119 (NaN)

Edp Sciences

Access to resources Recommend Favorite

Tomography of silicate dust around M-type AGB stars

By Bladh S.   Paladini C.   Höfner S.   Aringer B.  

Astronomy & Astrophysics, Vol. 607, Iss. issue, 2017-10 ,pp. : A27-A27 (NaN)

Edp Sciences

Access to resources Recommend Favorite