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M. Saberi

7 papers hereh-index 228 citations9 works total

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

author position
  • first author1
  • middle author5
  • last author1

Across the 7 of 7 papers where every author was matched, so the position is known.

fields
  • astro-ph.SR7
same name
  • M. Saberi — 16 papers, h 36
  • M. Saberi — 15 papers, h 7
  • M. Saberi — 6 papers, h 4
  • M. Saberi — 1 paper, h 2
  • M. Saberi — 1 paper, h 3
  • M. Saberi — 1 paper, h 3

Either other researchers who publish under this name, or the same person where the external sources have not merged their records.

identity via Semantic Scholar / OpenAlex

activity
20202026
most citedDEATHSTAR: Nearby AGB stars with the Atacama Compact Array II. CO envelope sizes and asymmetries: The S-type stars

12 citations · 15 across the 7 of their papers we have counts for

collaborators
Showing 2026Show all

3 papers · 1 filter

astro-ph.SR2026

A giant magnetic eruption from the asymptotic giant branch star Mira A

W. Vlemmings, M. Andriantsaralaza, B. Bojnordi Arbab +14

Mass loss during the advanced evolutionary stages of low- and intermediate-mass stars is traditionally attributed to dust-driven winds, whereas the influence of magnetic fields rem…

astro-ph.SR2026

The unique capabilities of HST for stellar physics: Probing Atmospheric Structure, Chromospheres, and Mass Loss of Evolved Stars

Maryam Saberi, Graham Harper, Jacco Th. van Loon +10

Evolved stars are among the primary sources of chemical enrichment and dust production in galaxies. During the giant phases, stars return a substantial fraction of their mass to th…

astro-ph.SR2026

A surprisingly large asymmetric ejection from Mira A

T. Khouri, W. H. T. Vlemmings, D. A. Raudales Oseguera +6

Stars with masses between roughly 1 and 8~M⊙​ end their lives on the asymptotic giant branch (AGB), when intense mass loss takes place. The outflows are generally accepted to…

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