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Sara Bladh

2 papers here

Matching runs newest-first, so older work may not be attached to this profile yet.

author position
  • first author1
  • last author1

Across the 2 of 2 papers where every author was matched, so the position is known.

fields
  • astro-ph.SR2
ORCID 0000-0003-2964-7943

identity via Semantic Scholar / OpenAlex

most citedExploring wind-driving dust species in cool luminous giants III. Wind models for M-type AGB stars: dynamic and photometric properties

67 citations · 116 across the 2 of their papers we have counts for

collaborators

2 papers

astro-ph.SR2016★ 49 cited

Constraining dust properties in Circumstellar Envelopes of C-stars in the Small Magellanic Cloud: optical constants and grain size of Carbon dust

Ambra Nanni, Paola Marigo, Martin A. T. Groenewegen +5

We present a new approach aimed at constraining the typical size and optical properties of carbon dust grains in Circumstellar envelopes (CSEs) of carbon-rich stars (C-stars) in th…

astro-ph.SR2015★ 67 cited

Exploring wind-driving dust species in cool luminous giants III. Wind models for M-type AGB stars: dynamic and photometric properties

S. Bladh, S. Höfner, B. Aringer +1

Stellar winds observed in asymptotic giant branch (AGB) stars are usually attributed to a combination of stellar pulsations and radiation pressure on dust. Shock waves triggered by…

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Not affiliated with arXiv. Researcher data from Semantic Scholar (ODC-BY) and OpenAlex.