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C. Sandín

3 papers here

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

author position
  • first author2
  • last author1

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

fields
  • astro-ph.GA2
  • astro-ph.SR1
ORCID 0000-0002-6370-5505

identity via Semantic Scholar / OpenAlex

most citedProperties of the three-dimensional structure in the central region of the supernova remnant SNR 0540-69.3

15 citations · 36 across the 3 of their papers we have counts for

collaborators

3 papers

astro-ph.SR2015★ 10 cited

Hot bubbles of planetary nebulae with hydrogen-deficient winds I. Heat conduction in a chemically stratified plasma

Christer Sandin, Matthias Steffen, Detlef Schönberner +1

Heat conduction has been found a plausible solution to explain discrepancies between expected and measured temperatures in hot bubbles of planetary nebulae (PNe). While the heat co…

astro-ph.GA2015★ 11 cited

Towards DIB mapping in galaxies beyond 100 Mpc. A radial profile of the λ5780.5 diffuse interstellar band in AM 1353-272 B

Ana Monreal-Ibero, Peter M. Weilbacher, Martin Wendt +5

Diffuse Interstellar Bands (DIBs) are non-stellar weak absorption features of unknown origin found in the spectra of stars viewed through one or several clouds of Interstellar Medi…

astro-ph.GA2013★ 15 cited

Properties of the three-dimensional structure in the central region of the supernova remnant SNR 0540-69.3

C. Sandin, P. Lundqvist, N. Lundqvist +3

We present and discuss new visual wavelength-range observations of the inner regions of the supernova remnant SNR 0540-69.3 that is located in the Large Magellanic Cloud (LMC). The…

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