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M. K. Andersen

3 papers hereh-index 364 citations6 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 3 papers where every author was matched, so the position is known.

fields
  • astro-ph.GA2
  • astro-ph.SR1

identity via Semantic Scholar / OpenAlex

activity
20132015
most citedGrain size limits derived from 3.6 μm and 4.5 μm coreshine

45 citations · 61 across the 2 of their papers we have counts for

collaborators

3 papers

astro-ph.SR2015★ 45 cited

Grain size limits derived from 3.6 μm and 4.5 μm coreshine

J. Steinacker, M. Andersen, W. -F. Thi +8

Recently discovered scattered light from molecular cloud cores in the wavelength range 3-5 μm (called "coreshine") seems to indicate the presence of grains with sizes above 0.5 μm.…

astro-ph.GA2014★ 16 cited

A common column density threshold for scattering at 3.6 mum and water-ice in molecular clouds

M. Andersen, W-F. Thi, J. Steinacker +1

Context: Observations of scattered light in the 1-5 μm range have revealed dust grains in molecular cores with sizes larger than commonly inferred for the diffuse interstellar me…

astro-ph.GA2013

Scattering from dust in molecular clouds: Constraining the dust grain size distribution through near-infrared cloudshine and infrared coreshine

M. Andersen, J. Steinacker, W-F. Thi +3

Context. The largest grains (0.5-1 micron) in the interstellar size distribution are efficient in scattering near- and mid-infrared radiation. These wavelengths are therefore parti…

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