activity
20202022
most citedExpanding bubbles in Orion A: [CII] observations of M42, M43, and NGC 1977

80 citations · 245 across the 7 of their papers we have counts for

collaborators

9 papers

astro-ph.GA202228 cited

FEEDBACK from the NGC7538 HII region

H. Beuther, N. Schneider, R. Simon +10

Context: How do expanding HII regions interact with their environmental cloud? This is one of the central questions driving the SOFIA legacy program FEEDBACK. Here, we present a ca…

astro-ph.IM202115 cited

Observation and calibration strategies for large-scale multi-beam velocity-resolved mapping of the [CII] emission in the Orion molecular cloud

R. Higgins, S. Kabanovic, C. Pabst +15

Context. The [CII] 158micron far-infrared fine-structure line is one of the dominant cooling lines of the star-forming interstellar medium (ISM). Hence [CII] emission originates in…

astro-ph.GA2021

[CII] line emission from Orion A. I. A template for extragalactic studies?

C. H. M. Pabst, A. Hacar, J. R. Goicoechea +10

The [CII] fine-structure line is one of the dominant coolants of the neutral interstellar medium. It is hence one of the brightest far-infrared emission lines an…

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.GA2021

SOFIA FEEDBACK survey: exploring the dynamics of the stellar wind driven shell of RCW 49

M. Tiwari, R. Karim, M. W. Pound +13

We unveil the stellar wind driven shell of the luminous massive star-forming region of RCW 49 using SOFIA FEEDBACK observations of the [CII] 158 m line. The complementary datase…

astro-ph.GA202062 cited

FEEDBACK: a SOFIA Legacy Program to Study Stellar Feedback in Regions of Massive Star Formation

N. Schneider, R. Simon, C. Guevara +37

FEEDBACK is a SOFIA legacy program dedicated to study the interaction of massive stars with their environment. It performs a survey of 11 galactic high mass star forming regions in…