English (United Kingdom)

https://curated-unify.zendy.io/wp-json/zendy-region/v1/featured_content/oa?rat=en

https://curated-unify.zendy.io/wp-json/zendy-region/v1/highlighted_journal/

Global: Zendy Plus annual

Presents the access of premium content as premium feature

Premium Content

Presents the keyphrase highlighting as premium feature

Keyphrase Highlighting

Presents the summarisation as premium feature

Summarisation

Insights

Presents the pdf analysis as premium feature

PDF Analysis

Presents the zaia usage as premium feature

ZAIA

Global: Zendy Tools annual

Global: Zendy Free Plan

Global: Zendy Tools monthly

Global: Zendy Plus monthly

A study has been conducted of 12C/13C ratios in five complex molecules in the Galactic center. H2CS, CH3CCH,\udNH2CHO, CH2CHCN, and CH3CH2CN and their 13C-substituted species have been observed in numerous\udtransitions at 1, 2, and 3 mm, acquired in a spectral-line survey of Sgr B2(N), conducted with the telescopes of the\udArizona Radio Observatory (ARO). Between 22 and 54 individual, unblended lines for the 12C species and 2–54\udfor 13C-substituted analogs were modeled in a global radiative transfer analysis. All five molecules were found\udto consistently exhibit two velocity components near VLSR ∼ 64 and 73 km s−1, with column densities ranging\udfrom Ntot ∼ 3 × 1014 − 4 × 1017 cm−2 and ∼2 × 1013 − 1 × 1017 cm−2 for the 12C and 13C species, respectively.\udBased on 14 different isotopic combinations, ratios were obtained in the range 12C/13C = 15 ± 5 to 33 ± 13, with\udan average value of 24 ± 7, based on comparison of column densities. These measurements better anchor the 12C/13C ratio at the Galactic center, and suggest a slightly revised isotope gradient of 12C/13C = 5.21(0.52) DGC +\ud22.6(3.3). As indicated by the column densities, no preferential 13C enrichment was found on the differing carbon\udsites of CH3CCH, CH2CHCN, and CH3CH2CN. Because of the elevated temperatures in Sgr B2(N), 13C isotopic\udsubstitution is effectively “scrambled,” diminishing chemical fractionation effects. The resulting ratios thus reflect\udstellar nucleosynthesis and Galactic chemical evolution, as is likely the case for most warm clouds

The12C/13C Ratio in Sgr B2(N): Constraints for Galactic Chemical Evolution and Isotopic Chemistry

The¹²C/¹³C Ratio in Sgr B2(N): Constraints for Galactic Chemical Evolution and Isotopic Chemistry