Nitrogen hydrides in the cold envelope of IRAS 16293-2422

Hily-Blant, P.; Maret, S.; Bacmann, A.; Bottinelli, S.; Parise, B.; Caux, E.; Faure, Alexandre; A. Bergin, Edwin; A. Blake, Geoffrey; Castets, A.; Ceccarelli, C.; Cernicharo, J.; Coutens, A.; Crimier, N.; Demyk, Karine; Dominik, C.; Gérin, Maryvonne; Hennebelle, P.; Henning, Thomas; Kahane, C.; Klotz, A.; Melnick, Gary; Pagani, L.; Schilke, P.; Vastel, C.; Wakelam, Valentine; Walters, Adam; Baudry, A.; Bell, Thomas; Benedettini, M.; C. A. Boogert, A.; Cabrit, S.; Caselli, P.; Codella, C.; Comito, C.; Encrenaz, P.; Falgarone, É.; Fuente, A.; F. Goldsmith, P.; Helmich, F.; Herbst, Eric; Jacq, T.; Kama, Mihkel; D. Langer, W.; Leflóch, B.; C. Lis, D.; Lord, S.; Lorenzani, A.; A. Neufeld, David; Nisini, B.; Pacheco, S.; G. Phillips, T.; Salez, M.; Saraceno, P.; Schüster, K.; Tielens, Xander; van der Tak, F.; H. D. van der Wiel, M.; Viti, S.; Wyrowski, F.; Yorke, H.

doi:10.1051/0004-6361/201015253

Public

Nitrogen hydrides in the cold envelope of IRAS 16293-2422

Published in Astronomy and Astrophysics • Sep 2, 2010

Authors:

P. Hily-Blant

S. Maret

A. Bacmann

Abstract

Nitrogen is the fifth most abundant element in the Universe, yet the gas-phase chemistry of N-bearing species remains poorly understood. Nitrogen hydrides are key molecules of nitrogen chemistry. Their abundance ratios place strong constraints on the production pathways and reaction rates of nitroge...

Subject

Protostar

Nitrogen

Submillimeter Array

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