most cited(Sub)stellar companions shape the winds of evolved stars

132 citations · 270 across the 6 of their papers we have counts for

collaborators

14 papers

astro-ph.SR2020132 cited

(Sub)stellar companions shape the winds of evolved stars

L. Decin, M. Montargès, A. M. S. Richards +32

Binary interactions dominate the evolution of massive stars, but their role is less clear for low- and intermediate-mass stars. The evolution of a spherical wind from an asymptotic…

astro-ph.GA202036 cited

Far-infrared laboratory spectroscopy of aminoacetonitrile and first interstellar detection of its vibrationally excited transitions

M. Melosso, A. Belloche, M. -A. Martin-Drumel +8

Aminoacetonitrile, a molecule detected in the interstellar medium only towards the star-forming region Sagittarius B2 (Sgr B2) thus far, is considered an important prebiotic specie…

astro-ph.GA202019 cited

Interstellar glycolamide: A comprehensive rotational study and an astronomical search in Sgr B2(N)

M. Sanz-Novo, A. Belloche, J. L. Alonso +6

Glycolamide is a glycine isomer and also one of the simplest derivatives of acetamide (e.g., one hydrogen atom is replaced with a hydroxyl group), which is a known interstellar mol…

astro-ph.SR2020

The ALMA-PILS survey: Inventory of complex organic molecules towards IRAS 16293-2422 A

S. Manigand, J. K. Jørgensen, H. Calcutt +6

Complex organic molecules (COM) are detected in many sources in the warm inner regions of envelopes surrounding deeply embedded protostars. Exactly how these COM form remains an op…

astro-ph.SR201926 cited

The ALMA-PILS survey: propyne (CHCCH) in IRAS 162932422

H. Calcutt, E. R. Willis, J. K. Jørgensen +7

Context. Propyne (CHCCH) has been detected in a variety of environments, from Galactic star-forming regions to extragalactic sources. Such molecules are excellent tracers of th…

astro-ph.GA201953 cited

The Physical and chemical structure of Sagittarius B2 -- IV. Converging filaments in the high-mass cluster forming region Sgr B2(N)

A. Schwörer, Á. Sánchez-Monge, P. Schilke +7

We have used an unbiased, spectral line-survey that covers the frequency range from 211 to 275 GHz and was obtained with ALMA (angular resolution of 0.4 arcsec) to study the small-…