📣 Help Shape the Future of UKRI's Gateway to Research (GtR)

We're improving UKRI's Gateway to Research and are seeking your input! If you would be interested in being interviewed about the improvements we're making and to have your say about how we can make GtR more user-friendly, impactful, and effective for the Research and Innovation community, please email gateway@ukri.org.

Detection of 15 NNH + in L1544: non-LTE modelling of dyazenilium hyperfine line emission and accurate 14 N/ 15 N values (2013)

First Author: Bizzocchi L

Attributed to: Star Formation and Protoplanetary Discs funded by STFC

Abstract

No abstract provided

Bibliographic Information

Digital Object Identifier: http://dx.doi.org/10.1051/0004-6361/201321276

Publication URI: http://dx.doi.org/10.1051/0004-6361/201321276

Type: Journal Article/Review

Parent Publication: Astronomy & Astrophysics

ISSN: 0004-6361