Pith. sign in

REVIEW 1 cited by

SO survey of massive cores

Not yet reviewed by Pith; the record is open.

Re-run · record.json Download PDF Read on arXiv ↗

This paper has not been read by Pith yet. Machine review is queued; the pith claim, tier, and objections will appear here once it completes.

SPECIMEN: schema-true, not a live event

T0 review · schema-true

One-sentence machine reading of the paper's core claim.

pith:XXXXXXXX · record.json · timestamp

arxiv 1711.09380 v1 pith:SM5EAP7S submitted 2017-11-26 astro-ph.GA

Igor Zinchenko (1) , Christian Henkel (2) ((1) Institute of Applied Physics of the Russian Academy of Sciences , Nizhny Novgorod , Russia , (2) Max-Planck-Institut fuer Radioastronomie , Bonn , Germany) This is my paper · ORCID
classification astro-ph.GA
keywords coressurveyabundancescolumndensedensitiesderivedeffelsberg
verification ladder T0 review T1 audit T2 compute T3 formal
0 comments
read the original abstract

We present the results of a survey of several tens of dense high mass star forming (HMSF) cores in three transitions of the SO molecule at 30 and 100 GHz with the 100-m Effelsberg and 20-m Onsala radio telescopes. The physical parameters of the cores are estimated from the line ratios and column densities. Relative abundances are derived as well.

Discussion (0). Continue with ORCID to comment.

Forward citations

Cited by 1 Pith paper

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Measuring Magnetic Field Strengths in Galactic Star-forming Regions via the Zeeman Effect with the SKA

    astro-ph.GA 2026-06 unverdicted novelty 2.0 of 10

    The paper presents predictions and observational plans for Zeeman effect measurements with SKA to provide statistical data on magnetic field strengths across scales in molecular clouds.

Pith tools