SIMBAD references

2018MNRAS.478.3693C - Mon. Not. R. Astron. Soc., 478, 3693-3720 (2018/August-2)

Nitrogen fractionation in high-mass star-forming cores across the Galaxy.

COLZI L., FONTANI F., RIVILLA V.M., SANCHEZ-MONGE A., TESTI L., BELTRAN M.T. and CASELLI P.

Abstract (from CDS):

The fractionation of nitrogen (N) in star-forming regions is a poorly understood process. To put more stringent observational constraints on the N-fractionation, we have observed with the IRAM-30-m telescope a large sample of 66 cores in massive star-forming regions. We targeted the (1-0) rotational transition of HN13C, HC15N, H13CN and HC15N, and derived the 14N/15N ratio for both HCN and HNC. We have completed this sample with that already observed by Colzi et al., and thus analysed a total sample of 87 sources. The 14N/15N ratios are distributed around the Proto-Solar Nebula value with a lower limit near the TA value (∼272). We have also derived the 14N/15N ratio as a function of the Galactocentric distance and deduced a linear trend based on unprecedented statistics. The Galactocentric dependences that we have found are consistent, in the slope, with past works but we have found a new local 14N/15N value of ∼400, i.e. closer to the Prosolar Nebula value. A second analysis was done, and a parabolic Galactocentric trend was found. Comparison with Galactic chemical evolution models shows that the slope until 8 kpc is consistent with the linear analysis, while the flattening trend above 8 kpc is well reproduced by the parabolic analysis.

Abstract Copyright: © 2018 The Author(s) Published by Oxford University Press on behalf of the Royal Astronomical Society

Journal keyword(s): stars: formation - stars: massive - ISM: abundances - ISM: molecules - primordial nucleosynthesis

VizieR on-line data: <Available at CDS (J/MNRAS/478/3693): table2.dat table3.dat tablea1.dat tablea2.dat tablea3.dat tablea4.dat>

Simbad objects: 74

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2023.01.31-10:32:45

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