The binary central star of the bipolar pre-planetary nebula IRAS 08005-2356 (V510 Pup)

Rajeev Manick, Brent Miszalski, Devika Kamath, Patricia Whitelock, Hans Van Winckel, Bruce J. Hrivnak, Brad N. Barlow, Shazrene Mohamed

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Abstract

Current models predict that binary interactions are a major ingredient in the formation of bipolar planetary nebulae (PNe) and pre-planetary nebulae (PPNe). Despite years of radial velocity (RV) monitoring, the paucity of known binaries amongst the latter systems means data are insufficient to examine this relationship in detail. In this work, we report on the discovery of a long-period (P = 2654 ± 124 d) binary at the centre of the Galactic bipolar PPN IRAS 08005-2356 (V510 Pup), determined from long-term spectroscopic and near-infrared time-series data. The spectroscopic orbit is fitted with an eccentricity of 0.36 ± 0.05, which is similar to that of other long-period post-AGB binaries. Time-resolved Hα profiles reveal high-velocity outflows (jets) with deprojected velocities up to 231+31−27 km s-1 seen at phases when the luminous primary is behind the jet. The outflow traced by Hα is likely produced via accretion on to a main-sequence companion, for which we calculate a mass of 0.63 ± 0.13 M. This discovery is one of the first cases of a confirmed binary PPN and demonstrates the importance of high-resolution spectroscopic monitoring surveys using large telescopes in revealing binarity among these systems.
Original languageEnglish
Pages (from-to)2226-2235
Number of pages10
JournalMonthly Notices of the Royal Astronomical Society
Volume508
Issue number2
DOIs
Publication statusPublished - Dec 2021

Bibliographical note

This article has been accepted for publication in Monthly Notices of the Royal Astronomical Society, Volume 508, Issue 2, December 2021, Pages 2226–2235, https://doi.org/10.1093/mnras/stab2428. Copyright 2021 The Author(s). Published by Oxford University Press on behalf of the Royal Astronomical Society. All rights reserved.

Keywords

  • techniques: photometric
  • techniques: spectroscopic
  • stars: AGB and post-AGB
  • binaries: spectroscopic
  • stars: evolution
  • stars: jets

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