nominal sky fibres

Discussion Cluster membership is solid in terms of concordant radial velocities to dRv<1 km/s, (especially given the steep sightline velocity gradient ), distance, CS, PN r eddening, location within the cluster boundary · 2011

1 Pith paper cite this work. Polarity classification is still indexing.

1 Pith paper citing it

browse 1 citing papers

representative citing papers

A high-mass Planetary Nebula in a Galactic Open Cluster

astro-ph.SR · 2019-06-25 · unverdicted · novelty 8.0

Planetary nebula BMP J1613-5406 is kinematically and spatially associated with NGC 6067, implying a progenitor mass of approximately 5 solar masses.

citing papers explorer

Showing 1 of 1 citing paper.

A high-mass Planetary Nebula in a Galactic Open Cluster astro-ph.SR · 2019-06-25 · unverdicted · none · ref 3
Planetary nebula BMP J1613-5406 is kinematically and spatially associated with NGC 6067, implying a progenitor mass of approximately 5 solar masses.

nominal sky fibres

fields

years

verdicts

representative citing papers

citing papers explorer