The puzzling high velocity G5 supergiant star HD 179821 : new insight from Gaia DR2 data

TL;DR

Using Gaia DR2 data, this study accurately determines the distance and evolutionary status of HD 179821, confirming it as a post-AGB star rather than a massive red supergiant, resolving longstanding debates.

Contribution

The paper provides the first precise distance measurement of HD 179821, clarifying its classification as a post-AGB star and refining its mass estimate, contrasting previous uncertain classifications.

Findings

HD 179821 is a post-AGB star with a mass around 0.8 Msun.

The star's distance is approximately 2959 parsecs.

It is not a 30 Msun red supergiant.

Abstract

HD 179821 is classified as G5 Ia star. From the IRAS colors and spectral energy distributions it was classified as a post-AGB star. But some studies classify it as a massive (30 to 19 Msun ) post-red supergiant evolving to become a Type II supernova. Its mass and evolutionary status remained a hotly debated question even after several detailed spectroscopic studies as the distance was not known. We use the parallax of HD 179821 from the second Gaia data release, and deduce its distance 2959 +/- 409 pc and its absolute magnitude MV = -5.7 +/- 0.3. Using the absolute magnitude determined in this paper, we show that HD 179821 fits very well with post-AGB tracks in the H-R diagram. Our results clearly confirm that HD 179821 is a post-AGB star of mass in the range of 0.8 Msun. It is not a 30 Msun red supergiant. The progenitor mass of this post-AGB star may be in the range of 4 Msun but may be a bit more.