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20072026
most citedATLASGAL --- properties of a complete sample of Galactic clumps

362 citations · 1.4k across the 46 of their papers we have counts for

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Showing 2019Show all

11 papers · 1 filter

astro-ph.GA201912 cited

SPARKS II.: Complex organic molecules in accretion shocks around a hot core precursor

T. Csengeri, A. Belloche, S. Bontemps +3

Classical hot cores are rich in molecular emission, and they show a high abundance of complex organic molecules (COMs). The emergence of molecular complexity is poorly constrained…

astro-ph.SR201953 cited

Chemical complexity in high-mass star formation: An observational and modeling case study of the AFGL 2591 VLA 3 hot core

C. Gieser, D. Semenov, H. Beuther +30

We present a detailed observational and modeling study of the hot core VLA 3 in the high-mass star-forming region AFGL 2591, which is a target region of the NOrthern Extended Milli…

astro-ph.SR2019

An ALMA Study of the FU-Ori Type Object V900 Mon: Implications for the Progenitor

Michihiro Takami, Tsu-Sheng Chen, Hauyu Baobab Liu +13

We present ALMA observations of 12CO, 13CO, and C18O J=2--1 lines and the 230 GHz continuum for the FU Ori-type object (FUor) V900 Mon (d~1.5 kpc), for which the accretion burst wa…

astro-ph.GA2019

Fragmentation and filaments at the onset of star and cluster formation: SABOCA 350 m view of ATLASGAL selected massive clumps

Yuxin Lin, Timea Csengeri, Friedrich Wyrowski +4

The structure formation of the dense interstellar material and the fragmentation of clumps into cores is a fundamental step to understand how stars and stellar clusters form. We ai…

astro-ph.SR2019

Dense cores and star formation in the giant molecular cloud Vela~C

F. Massi, A. Weiss, D. Elia +12

Context The Vela Molecular Ridge is one of the nearest (700 pc) giant molecular cloud (GMC) complexes hosting intermediate-mass (up to early B, late O stars) star formation, and is…

astro-ph.GA20199 cited

Probing the initial conditions of high-mass star formation. III. Fragmentation and triggered star formation

Chuan-Peng Zhang, Timea Csengeri, Friedrich Wyrowski +6

Massive clumps tend to fragment into clusters of cores and condensations, some of which form high-mass stars. In this work, we study the structure of massive clumps at different sc…