SIMBAD references

2018MNRAS.477.2243R - Mon. Not. R. Astron. Soc., 477, 2243-2250 (2018/June-3)

Distances to supernova remnants G20.4 + 0.1, G24.7 - 0.6, and G28.6 - 0.1 and new molecular cloud associations.

RANASINGHE S. and LEAHY D.A.

Abstract (from CDS):

Accurate distances to supernova remnants (SNRs) are crucial in determining their size, age, luminosity, and evolutionary state. To determine distances, we chose three SNRs from the VLA (Very Large Array) Galactic Plane Survey for extraction of H I absorption spectra. Analysing H I absorption spectra, 13CO emission spectra, and H I and 13CO channel maps, kinematic velocities (or their limits) to the three SNRs were calculated. The three SNRs are probably associated with molecular clouds and the new distance to G20.4 + 0.1, G24.7 - 0.6, and G28.6 - 0.1 are 7.8 ± 0.5 kpc, 3.8 ± 0.2 kpc, and 9.6 ± 0.3 kpc, respectively.

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

Journal keyword(s): ISM: supernova remnants - radio continuum: ISM - radio lines: ISM

Simbad objects: 7

goto Full paper

goto View the reference in ADS

To bookmark this query, right click on this link: simbad:2018MNRAS.477.2243R and select 'bookmark this link' or equivalent in the popup menu


2020.09.26-07:27:46

© Université de Strasbourg/CNRS

    • Contact