activity
20212023
most citedSelf-absorption in [CII], CO, and HI in RCW120. Building up a geometrical and physical model of the region

33 citations · 67 across the 5 of their papers we have counts for

collaborators

5 papers

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.GA20232 cited

Structure of the W3A Low Density Foreground Region

Paul F. Goldsmith, William D. Langer, Youngmin Seo +5

We present analysis of OI 63 micron and CO = 5-4 and 8-7 multi-position data in the W3A region and use it to develop a model for the extended low-density foreground gas that pr…

astro-ph.GA20228 cited

SOFIA FEEDBACK survey: PDR diagnostics of stellar feedback in different regions of RCW 49

M. Tiwari, M. Wolfire, M. W. Pound +13

We quantified the effects of stellar feedback in RCW 49 by determining the physical conditions in different regions using the [CII] 158 m and [OI] 63 m observations from SOFI…

astro-ph.GA202224 cited

The SOFIA FEEDBACK Legacy Survey: Dynamics and mass ejection in the bipolar HII region RCW 36

L. Bonne, N. Schneider, P. García +20

We present [CII] 158 m and [OI] 63 m observations of the bipolar HII region RCW 36 in the Vela C molecular cloud, obtained within the SOFIA legacy project FEEDBACK, which is…

astro-ph.GA202133 cited

Self-absorption in [CII], CO, and HI in RCW120. Building up a geometrical and physical model of the region

S. Kabanovic, N. Schneider, V. Ossenkopf-Okada +19

Revealing the 3D dynamics of HII regions and their associated molecular clouds is important for understanding the longstanding problem as to how stellar feedback affects the densit…