The Gaia Data Release 1 parallaxes and the distance scale of Galactic planetary nebulae

Abstract

In this paper we gauge the potentiality of Gaia in the distance scale calibration of planetary nebulae (PNe) by assessing the impact of DR1 parallaxes of central stars of Galactic PNe (CSPNe) against known physical relations. For selected PNe targets with state-of-the-art data on angular sizes and fluxes, we derive the distance-dependent parameters of the classical distance scales, i.e., physical radii and ionized masses, from DR1 parallaxes; we propagate the uncertainties in the estimated quantities and evaluate their statistical properties in the presence of large relative parallax errors; we populate the statistical distance scale diagrams with this sample and discuss its significance in light of existing data and current calibrations. We glean from DR1 parallaxes 8 CSPNe with S/N$>$1. We show that this set of potential calibrators doubles the number of extant trigonometric parallaxes (from HST and ground-based), and increases by two orders of magnitude the domain of physical parameters probed previously. We then use the combined sample of suitable trigonometric parallaxes to fit the physical-radius-to-surface-brightness relation. This distance scale calibration, although preliminary, appears solid on statistical grounds, and suggestive of new PNe physics. With the tenfold improvement in PNe number statistics and astrometric accuracy expected from future Gaia releases the new distance scale, already very intriguing, will be definitively constrained.

arXiv commentNew Astronomy, in press

References in corpus (20)

• Gaia Data Release 1. Summary of the astrometric, photometric, and survey properties
• Gaia Data Release 1: Astrometry - one billion positions, two million proper motions and parallaxes
• On the Galactic Disk Metallicity Distribution from Open Clusters I. New Catalogues and Abundance Gradient
• The Hα surface brightness - radius relation: a robust statistical distance indicator for planetary nebulae
• A Hubble Space Telescope Survey for Resolved Companions of Planetary-Nebula Nuclei
• The Tycho-Gaia astrometric solution. How to get 2.5 million parallaxes with less than one year of Gaia data
• The Galactic structure and chemical evolution traced by the population of planetary nebulae
• The Magellanic Cloud Calibration of the Galactic Planetary Nebula Distance Scale
• Trigonometric Parallaxes of Central Stars of Planetary Nebulae
• A catalogue of integrated H-alpha fluxes for 1,258 Galactic planetary nebulae
• The binary fraction of planetary nebula central stars I. A high-precision, I-band excess search
• New light on Galactic post-asymptotic giant branch stars. I. First distance catalogue
• A test of Gaia Data Release 1 parallaxes: implications for the local distance scale
• Hubble Space Telescope Observations of the Planetary Nebula K648 in the Globular Cluster M15
• Observations and three-dimensional ionization structure of the planetary nebula SuWt 2
• Chemical Abundances and Dust in the Halo Planetary Nebula K648 in M15: Its Origin and Evolution based on an Analysis of Multiwavelength Data
• Spectral analysis of BD+30${}^{\circ }$623, the peculiar binary central star of the planetary nebula NGC 1514
• The Exotic Eclipsing Nucleus of the Ring Planetary Nebula SuWt2
• On the distances of planetary nebulae
• The two central stars of NGC 1514: can they actually be related?

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• A young multipolar planetary nebula in the making: IRAS 21282+5050
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