◍wovepaper
SearchResearchersInstitutions
Sign in
researcher

M. Röllig

4 papers hereh-index 13804 citations41 works total

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

author position
  • first author1
  • middle author3

Across the 4 of 4 papers where every author was matched, so the position is known.

fields
  • astro-ph2
  • astro-ph.GA1
  • astro-ph.IM1
same name
  • M. Röllig — 30 papers, h 17
  • M. Röllig — 14 papers, h 15
  • M. Röllig — 7 papers
  • M. Röllig — 7 papers, h 0
  • M. Röllig — 6 papers, h 9
  • M. Röllig — 3 papers

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
20082021
most citedFull SED fitting with the KOSMA-τ PDR code - I. Dust modelling

48 citations · 100 across the 4 of their papers we have counts for

collaborators

4 papers

astro-ph.GA2021

Stellar feedback and triggered star formation in the prototypical bubble RCW 120

Matteo Luisi, Loren D. Anderson, Nicola Schneider +17

Radiative and mechanical feedback of massive stars regulates star formation and galaxy evolution. Positive feedback triggers the creation of new stars by collecting dense shells of…

astro-ph.IM2012★ 48 cited

Full SED fitting with the KOSMA-τ PDR code - I. Dust modelling

M. Röllig, R. Szczerba, V. Ossenkopf +1

We revised the treatment of interstellar dust in the KOSMA-τ PDR model code to achieve a consistent description of the dust-related physics in the code. The detailed knowledge of t…

astro-ph2008★ 16 cited

The Photon Dominated Region in the IC 348 molecular cloud

K. Sun, V. Ossenkopf, C. Kramer +4

In this paper we discuss the physical conditions of clumpy nature in the IC 348 molecular cloud. We combine new observations of fully sampled maps in [C I] at 492 GHz and 12CO 4--3…

astro-ph2008★ 36 cited

Submillimeter Line Emission from LMC N159W: a Dense, Clumpy PDR in a Low Metallicity Environment

J. L. Pineda, N. Mizuno, J. Stutzki +30

Star formation at earlier cosmological times takes place in an interstellar medium with low metallicity. The Large Magellanic Cloud (LMC) is ideally suited to study star formation…

◍wovepaper

Papers, researchers and institutions, woven together.

Explore
  • Search
  • Researchers
  • Institutions
Account
  • Library
  • Chat
Data
  • arXiv.org
  • Semantic Scholar
  • OpenAlex
  • Latest RSS
AboutContactPrivacyDevelopersllms.txtopenapi.json
Not affiliated with arXiv. Researcher data from Semantic Scholar (ODC-BY) and OpenAlex.