Kris Davidson, Greta Helmel, Roberta M. Humphreys
Published 2018-08-06Version 1
Gaia parallaxes for the star cluster Tr 16 reveal a discrepancy in the oft-quoted distance of Eta Carinae. It is probably more distant and more luminous. Moreover, many presumed members may not belong to Tr 16.
Comments: This article is nearly identical to AAS Research Note: RNAAS 2:133, 2018 Aug 1
Journal: RNAAS 2:133, 2018
Dynamical masses of Cepheids from the GAIA parallaxes
Long-term evolution in ionization of ejecta illuminated by Eta Carinae
Multi-Wavelength Implications of the Companion Star in Eta Carinae
![QR code for arXiv:1808.02073 [astro-ph.SR]](http://oss.arxitics.com/images/favicon.svg)