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researcher

S. Wolf

21 papers hereh-index 16711 citations19 works total

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

author position
  • middle author11
  • last author9

Across the 20 of 21 papers where every author was matched, so the position is known.

fields
  • astro-ph.SR13
  • astro-ph.EP7
  • astro-ph.GA1
same name
  • S. Wolf — 122 papers, h 39
  • S. Wolf — 58 papers, h 37
  • S. Wolf — 29 papers, h 38
  • S. Wolf — 13 papers, h 10
  • S. Wolf — 11 papers, h 7
  • S. Wolf — 10 papers, h 4

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
20102023
most citedDUst Around NEarby Stars. The survey observational results

220 citations · 1k across the 20 of their papers we have counts for

collaborators
Showing 2017Show all

4 papers · 1 filter

astro-ph.SR2017★ 31 cited

Magnetic fields in circumstellar disks: The potential of Zeeman observations

R. Brauer, S. Wolf, M. Flock

Context. Recent high angular resolution polarimetric continuum observations of circumstellar disks provide new insights into their magnetic field. However, direct constraints are l…

astro-ph.EP2017★ 27 cited

Collisions and drag in debris discs with eccentric parent belts

T. Löhne, A. V. Krivov, F. Kirchschlager +2

Context: High-resolution images of circumstellar debris discs reveal off-centred rings that indicate past or ongoing perturbation, possibly caused by secular gravitational interact…

astro-ph.SR2017★ 33 cited

The origin of dust polarization in molecular outflows

S. Reissl, D. Seifried, S. Wolf +2

Aims: In this paper we present a case study to investigate conditions necessary to detect a characteristic magnetic field substructure embedded in a large-scale field. A helical ma…

astro-ph.GA2017★ 36 cited

Magnetic fields in molecular clouds: Limitations of the analysis of Zeeman observations

R. Brauer, S. Wolf, S. Reissl +1

Context. Observations of Zeeman split spectral lines represent an important approach to derive the structure and strength of magnetic fields in molecular clouds. In contrast to the…

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