The canonical Luminous Blue Variable AG Car and its neighbor Hen 3-519 are much closer than previously assumed
Nathan Smith (1), Keivan G. Stassun (2,3) ((1) University of, Arizona, (2) Vanderbilt University, (3) Fisk University)

TL;DR
This study uses Gaia data to measure distances to key LBVs, revealing they are closer and less luminous than previously thought, which impacts their evolutionary understanding and potential as supernova progenitors.
Contribution
First direct Gaia-based distance measurements for several canonical LBVs, challenging previous assumptions about their luminosities and evolutionary states.
Findings
AG Car and Hen 3-519 are closer than previously assumed.
Lower luminosities suggest past red supergiant phases.
Implications for LBV evolution and supernova progenitor models.
Abstract
The strong mass loss of Luminous Blue Variables (LBVs) is thought to play a critical role in massive-star evolution, but their place in the evolutionary sequence remains debated. A key to understanding their peculiar instability is their high observed luminosities, which often depends on uncertain distances. Here we report direct distances and space motions of four canonical Milky Way LBVs---AG~Car, HR~Car, HD~168607, and (candidate) Hen~3-519---from the Gaia first data release. Whereas the distances of HR~Car and HD~168607 are consistent with previous literature estimates within the considerable uncertainties, Hen~3-519 and AG~Car, both at 2~kpc, are much closer than the 6--8~kpc distances previously assumed. As a result, Hen~3-519 moves far from the locus of LBVs on the HR Diagram, making it a much less luminous object. For AG~Car, considered a defining example of a classical…
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
