K.M. Menten
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View article: Molecular clouds at the edge of the Galaxy
Molecular clouds at the edge of the Galaxy Open
The Galactic edge, at Galactocentric distances of 14–22 kpc, provides an ideal laboratory for studying molecular clouds in an environ-ment that is different from the solar neighborhood, due to its lower gas density, lower metallicity, and …
View article: Time evolution of o-H<sub>2</sub>D<sup>+</sup>, N<sub>2</sub>D<sup>+</sup>, and N<sub>2</sub>H<sup>+</sup> during the high-mass star formation process
Time evolution of o-H<sub>2</sub>D<sup>+</sup>, N<sub>2</sub>D<sup>+</sup>, and N<sub>2</sub>H<sup>+</sup> during the high-mass star formation process Open
Context . Deuterium fractionation is a well-established evolutionary tracer in low-mass star formation, but its applicability to the high-mass regime remains an open question. In this context, the abundances and ratios of different deutera…
View article: High-resolution observations of <sup>12</sup>CO and <sup>13</sup>CO <i>J</i> = 3 → 2 towards the NGC 6334 extended filament
High-resolution observations of <sup>12</sup>CO and <sup>13</sup>CO <i>J</i> = 3 → 2 towards the NGC 6334 extended filament Open
NGC 6334 is a giant molecular cloud (GMC) complex that exhibits elongated filamentary structure and harbours numerous OB-stars, H II regions, and star-forming clumps. To study the emission morphology and velocity structure of the gas in th…
View article: Physical and chemical structure of high-mass star-forming regions
Physical and chemical structure of high-mass star-forming regions Open
Aims. Current star formation research centers the characterization of the physical and chemical properties of massive stars, which are in the process of formation, at the spatial resolution of individual high-mass cores. Methods. We use su…
View article: Chemical complexity in high-mass star formation: An observational and modeling case study of the AFGL 2591 VLA 3 hot core
Chemical complexity in high-mass star formation: An observational and modeling case study of the AFGL 2591 VLA 3 hot core Open
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 Millimeter Array (NOEMA) large program CORE. Using NOEMA observa…