The ALMA-PILS survey: First detection of nitrous acid (HONO) in the interstellar medium
Artikel i vetenskaplig tidskrift, 2019

Nitrogen oxides are thought to play a significant role as a nitrogen reservoir and to potentially participate in the formation of more complex species. Until now, only NO, NO, and HNO have been detected in the interstellar medium. We report the first interstellar detection of nitrous acid (HONO). Twelve lines were identified towards component B of the low-mass protostellar binary IRAS 16293-2422 with the Atacama Large Millimeter/submillimeter Array, at the position where NO and NO have previously been seen. A local thermodynamic equilibrium model was used to derive the column density (∼9 × 1014 cm in a 0 .″5 beam) and excitation temperature (∼100 K) of this molecule. HNO, NO, NO+, and HNO3 were also searched for in the data, but not detected. We simulated the HONO formation using an updated version of the chemical code Nautilus and compared the results with the observations. The chemical model is able to reproduce satisfactorily the HONO, NO, and NO abundances, but not the NO, HNO, and NHOH abundances. This could be due to some thermal desorption mechanisms being destructive and therefore limiting the amount of HNO and NHOH present in the gas phase. Other options are UV photodestruction of these species in ices or missing reactions potentially relevant at protostellar temperatures.

Stars

Astrochemistry

protostars

individual objects

Stars

molecules

ISM

IRAS 16293-2422

ISM

formation

Författare

A. Coutens

Université de Bordeaux

N. F W Ligterink

Universität Bern

J. C. Loison

Université de Bordeaux

V. Wakelam

Université de Bordeaux

Hannah Calcutt

Chalmers, Rymd-, geo- och miljövetenskap, Astronomi och plasmafysik, Galaktisk astrofysik

M. N. Drozdovskaya

Universität Bern

Jes K. Jørgensen

Köpenhamns universitet

H. S.P. Müller

Universität zu Köln

E. F. van Dishoeck

Universiteit Leiden

Max Planck-institutet

S. F. Wampfler

Universität Bern

Astronomy and Astrophysics

0004-6361 (ISSN) 1432-0746 (eISSN)

Vol. 623 L13

Ämneskategorier

Astronomi, astrofysik och kosmologi

Atom- och molekylfysik och optik

Annan kemi

DOI

10.1051/0004-6361/201935040

Mer information

Senast uppdaterat

2019-04-29