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B. Larsson

34 papers hereh-index 272.8k citations101 works total

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

author position
  • first author4
  • middle author14
  • last author3

Across the 21 of 34 papers where every author was matched, so the position is known.

fields
  • astro-ph.GA18
  • astro-ph7
  • astro-ph.SR5
  • astro-ph.EP3
  • astro-ph.IM1
same name
  • B. Larsson — 14 papers, h 9
  • B. Larsson — 5 papers, h 3
  • B. Larsson — 1 paper, h 2

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
20032021
most citedWater in Star-Forming Regions with the Herschel Space Observatory (WISH): Overview of key program and first results

262 citations · 2.1k across the 34 of their papers we have counts for

collaborators
Showing 2015 · astro-ph.GAShow all

3 papers · 2 filters

astro-ph.GA2015★ 12 cited

Herschel HIFI Observations of the Sgr A +50 km/s Cloud. Deep Searches for O2 in Emission and Foreground Absorption

Aa. Sandqvist, B. Larsson, Å. Hjalmarson +8

To date O2 has definitely been detected in only two sources, namely rho Oph A and Orion, reflecting the extremely low abundance of O2 in the interstellar medium. One of the sources…

astro-ph.GA2015★ 5 cited

Search for HOOH in Orion

René Liseau, Bengt Larsson

Context: The abundance of key molecules determines the level of cooling that is necessary for the formation of stars and planetary systems. In this context, one needs to understand…

astro-ph.GA2015

Gas and dust in the star-forming region rho Oph A: The dust opacity exponent beta and the gas-to-dust mass ratio g2d

R. Liseau, B. Larsson, T. Lunttila +6

We aim at determining the spatial distribution of the gas and dust in star-forming regions and address their relative abundances in quantitative terms. We also examine the dust opa…

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