NGC 2022, a case study of a multiple-shell planetary nebula

B. Montoro-Molina, M. A. Guerrero, E. Santamaría, J. A. Toalá, Y. H. Chu, G. Ramos-Larios, R. Infante-Sainz, M. Akhlaghi, S. Eskandarlou, C. López-Sanjuan

Research output: Contribution to journalArticlepeer-review

Abstract

We present a detailed study of the physical properties, history of mass loss, and chemical abundances of the planetary nebula NGC 2022. New imaging observations obtained with the OAJ/JAST80 and NOT/ALFOSC confirm the presence of a faint ∼88 arcsec halo surrounding a double-layered elliptical structure that consists of a bright 21.4 × 16.7 arcsec inner shell and a 32 arcsec diameter envelope. The long-slit high-dispersion echelle observations obtained with MES on the OAN-SPM 2.1-m telescope can be well described by a shape model with expansion velocities of 43 ± 3 and 34 ± 3 km s-1 along the major and minor axes of the elliptical inner shell, respectively. In addition, a deep long-slit high-dispersion echelle observation made with the KPNO 4-m telescope detected line-splitting in the faint halo, revealing an expansion velocity of 15.5 ± 2 km s-1. We have also used new intermediate-dispersion optical spectra with the NOT, complemented with IUE data, to study the chemical abundances of each shell. The abundances of the three shells are typical of a Type II in the Peimbert classification of PNe and do not exhibit any notable anomalies. Finally, we estimate the total mass of NGC 2022 to be ≈0.9 M⊙>, which consists of 0.64 M⊙> from the CSPN and 0.1, 0.11, and 0.1 × M⊙> from the ionized inner shell, outer shell, and halo, respectively.

Original languageEnglish (US)
Pages (from-to)1601-1614
Number of pages14
JournalMonthly Notices of the Royal Astronomical Society
Volume524
Issue number2
DOIs
StatePublished - Sep 1 2023
Externally publishedYes

Keywords

  • (ISM:) planetary nebulae: general
  • (ISM:) planetary nebulae: individual: (NGC 2022)
  • stars: evolution

ASJC Scopus subject areas

  • Astronomy and Astrophysics
  • Space and Planetary Science

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