activity
20102024
most citedDetection of interstellar oxidaniumyl: abundant H2O+ towards the star-forming regions DR21, Sgr B2, and NGC6334

87 citations · 230 across the 8 of their papers we have counts for

collaborators

8 papers

astro-ph.GA2024★ 1 cited

Description of turbulent dynamics in the interstellar medium: Multifractal microcanonical analysis: II. Sparse filtering of Herschel observation maps and visualization of filamentary structures at different length scales

A. Rashidi, H. Yahia, S. Bontemps +15

We present significant improvements to our previous work on noise reduction in {\sl Herschel} observation maps by defining sparse filtering tools capable of handling, in a unified…

astro-ph.GA2024

First detection of the [CII] 158 micron line in the intermediate-velocity cloud Draco

N. Schneider, V. Ossenkopf-Okada, E. Keilmann +7

High-latitude intermediate-velocity clouds (IVCs) are part of the Milky Way's HI halo and originate from either a galactic fountain process or extragalactic gas infall. They are pa…

astro-ph.GA2023★ 17 cited

The SOFIA FEEDBACK Legacy Survey: Rapid molecular cloud dispersal in RCW 79

L. Bonne, S. Kabanovic, N. Schneider +12

It has long been discussed whether stellar feedback in the form of winds and/or radiation can shred the nascent molecular cloud, thereby controlling the star formation rate. Howeve…

astro-ph.GA2023

Identifying physical structures in our Galaxy with Gaussian Mixture Models: An unsupervised machine learning technique

M. Tiwari, R. Kievit, S. Kabanovic +14

We explore the potential of the Gaussian Mixture Model (GMM), an unsupervised machine learning method, to identify coherent physical structures in the ISM. The implementation we pr…

astro-ph.GA2020★ 50 cited

Formation of the Musca filament: Evidence for asymmetries in the accretion flow due to a cloud-cloud collision

L. Bonne, S. Bontemps, N. Schneider +11

Context. Dense molecular filaments are ubiquituous in the interstellar medium, yet their internal physical conditions and formation mechanism remain debated. Aims. We study the kin…

astro-ph.GA2010★ 51 cited

Strong CH+ J=1-0 emission and absorption in DR21

E. Falgarone, V. Ossenkopf, M. Gerin +30

We report the first detection of the ground-state rotational transition of the methylidyne cation CH+ towards the massive star-forming region DR21 with the HIFI instrument onboard…

astro-ph.GA2010★ 87 cited

Detection of interstellar oxidaniumyl: abundant H2O+ towards the star-forming regions DR21, Sgr B2, and NGC6334

V. Ossenkopf, H. S. P. Müller, D. C. Lis +99

We identify a prominent absorption feature at 1115 GHz, detected in first HIFI spectra towards high-mass star-forming regions, and interpret its astrophysical origin. The character…

astro-ph.GA2010★ 24 cited

HIFI observations of warm gas in DR21: Shock versus radiative heating

V. Ossenkopf, M. Röllig, R. Simon +35

The molecular gas in the DR21 massive star formation region is known to be affected by the strong UV field from the central star cluster and by a fast outflow creating a bright sho…