SIMBAD references

2015ApJ...808L..46F - Astrophys. J., 808, L46 (2015/August-1)

First measurements of 15N fractionation in N2H+ toward high-mass star-forming cores.

FONTANI F., CASELLI P., PALAU A., BIZZOCCHI L. and CECCARELLI C.

Abstract (from CDS):

We report on the first measurements of the isotopic ratio 14N/15N in N2H+ toward a statistically significant sample of high-mass star-forming cores. The sources belong to the three main evolutionary categories of the high-mass star formation process: high-mass starless cores, high-mass protostellar objects, and ultracompact H ii regions. Simultaneous measurements of the 14N/15N ratio in CN have been made. The 14N/15N ratios derived from N2H+ show a large spread (from ∼180 up to ∼1300), while those derived from CN are in between the value measured in the terrestrial atmosphere (∼270) and that of the proto-solar nebula (∼440) for the large majority of the sources within the errors. However, this different spread might be due to the fact that the sources detected in the N2H+ isotopologues are more than those detected in the CN ones. The 14N/15N ratio does not change significantly with the source evolutionary stage, which indicates that time seems to be irrelevant for the fractionation of nitrogen. We also find a possible anticorrelation between the 14N/15N (as derived from N2H+) and the H/D isotopic ratios. This suggests that 15N enrichment could not be linked to the parameters that cause D enrichment, in agreement with the prediction by recent chemical models. These models, however, are not able to reproduce the observed large spread in 14N/15N, pointing out that some important routes of nitrogen fractionation could be still missing in the models.

Abstract Copyright:

Journal keyword(s): ISM: molecules - molecular data - radio lines: ISM - stars: formation - submillimeter: ISM

Simbad objects: 26

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2020.09.19-01:25:50

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