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M. Firnstein

4 papers hereh-index 4210 citations13 works total

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

author position
  • first author2
  • middle author1

Across the 3 of 4 papers where every author was matched, so the position is known.

fields
  • astro-ph2
  • astro-ph.SR2
same name
  • M. Firnstein — 2 papers

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
20062012
most citedLMC origin of the hyper-velocity star HE 0437-5439. Beyond the supermassive black hole paradigm

62 citations · 107 across the 4 of their papers we have counts for

collaborators

4 papers

astro-ph.SR2012★ 45 cited

Quantitative spectroscopy of Galactic BA-type supergiants. I. Atmospheric parameters

M. Firnstein, N. Przybilla

BA-type supergiants show a high potential as versatile indicators for modern astronomy. The focus here is on the determination of accurate and precise atmospheric parameters for a…

astro-ph.SR2009

Tepid Supergiants: Chemical Signatures of Stellar Evolution & The Extent of Blue Loops

Norbert Przybilla, Markus Firnstein, Maria-Fernanda Nieva

Massive stars can develop into tepid supergiants at several stages of their post main-sequence evolution, prior to core He-burning, on a blue loop, or close to the final supernova…

astro-ph2008★ 62 cited

LMC origin of the hyper-velocity star HE 0437-5439. Beyond the supermassive black hole paradigm

N. Przybilla, M. F. Nieva, U. Heber +4

Context: Hyper-velocity stars move so fast that only a supermassive black hole (SMBH) seems to be capable to accelerate them. Hence the Galactic centre (GC) is their only suggested…

astro-ph2006

CNO Abundances of BA-Type Supergiants

M. Firnstein, N. Przybilla

Massive BA-type supergiants are among the visually brightest stars in galaxies with active star formation. As such they are versatile tools for studies of stellar and galactochemic…

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