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researcher

M. Juvela

319 papers hereh-index 8139.3k citations459 works total

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

author position
  • sole author8
  • first author31
  • middle author154
  • last author12

Across the 205 of 319 papers where every author was matched, so the position is known.

fields
  • astro-ph.GA182
  • astro-ph.CO66
  • astro-ph45
  • astro-ph.IM20
  • astro-ph.SR6
same name
  • M. Juvela — 16 papers
  • M. Juvela — 1 paper, h 7
  • M. Juvela — 1 paper, h 0
  • M. Juvela — 1 paper, h 1

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
19972026
most citedPlanck 2013 results. XVI. Cosmological parameters

6.6k citations · 32.9k across the 318 of their papers we have counts for

collaborators
Showing 2010Show all

4 papers · 1 filter

astro-ph.GA2010★ 19 cited

Physical properties of dense cores in Orion B9

Oskari Miettinen, Jorma Harju, Lauri K. Haikala +1

We aim to determine the physical and chemical properties of dense cores in Orion B9. We observed the NH3(1,1) and (2,2), and the N2H+(3-2) lines towards the submm peak positions. T…

astro-ph.GA2010★ 89 cited

Accuracy of core mass estimates in simulated observations of dust emission

J. Malinen, M. Juvela, D. C. Collins +2

We study the reliability of mass estimates obtained for molecular cloud cores using sub-millimetre and infrared dust emission. We use magnetohydrodynamic simulations and radiative…

astro-ph.GA2010★ 806 cited

Clouds, filaments and protostars: the Herschel Hi-GAL Milky Way

S. Molinari, B. Swinyard, J. Bally +121

We present the first results from the science demonstration phase for the Hi-GAL survey, the Herschel key-project that will map the inner Galactic Plane of the Milky Way in 5 bands…

astro-ph.GA2010★ 10 cited

Scattered H-alpha emission from a large translucent cloud G294-24

K. Lehtinen, M. Juvela, K. Mattila

We study an undocumented large translucent cloud, detected by means of its enhanced radiation on the SHASSA (Southern H-Alpha Sky Survey Atlas) survey. We consider whether its exce…

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