Ancient `ghost' planetary nebulae discovered with amateur telescopes

As planetary nebulae evolve, they fade and dissipate into the surrounding interstellar medium, which makes them harder to detect. Modern, advanced amateur equipment can help to uncover this hidden population of ancient `ghost' planetary nebulae. Via careful processing of long-integration, narrow-band imagery with modest aperture telescopes at a dark-sky site, we detected three new candidate planetary nebulae (JAM 2, JAM 3, and JAM 4). Each measures several arcminutes across with O iii surface brightnesses of order 30 mag arcsec -2 . For each nebula, we identify a candidate central star, the parallaxes of which lead to nebular age estimates in the range 50--100 thousand years. The candidate central star of JAM 2 also shows indications of photometric variability, potentially due to spots on the stellar surface.

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Publication Details

Journal
Springer Link (Chiba Institute of Technology)
Published
2026-04-24
DOI
https://doi.org/10.1051/0004-6361/202659488/pdf
Primary Topic
Stellar, planetary, and galactic studies
Type
article
Field-Weighted Citation Impact
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article

Ancient `ghost' planetary nebulae discovered with amateur telescopes

J. A. Manuel, M. Santander-García, D. Jones, N. Reindl
Springer Link (Chiba Institute of Technology)
Stellar, planetary, and galactic studies
article

Ancient `ghost' planetary nebulae discovered with amateur telescopes

J. A. Manuel, M. Santander-García, D. Jones, N. Reindl
article en

Abstract

As planetary nebulae evolve, they fade and dissipate into the surrounding interstellar medium, which makes them harder to detect. Modern, advanced amateur equipment can help to uncover this hidden population of ancient `ghost' planetary nebulae. Via careful processing of long-integration, narrow-band imagery with modest aperture telescopes at a dark-sky site, we detected three new candidate planetary nebulae (JAM 2, JAM 3, and JAM 4). Each measures several arcminutes across with O iii surface brightnesses of order 30 mag arcsec -2 . For each nebula, we identify a candidate central star, the parallaxes of which lead to nebular age estimates in the range 50--100 thousand years. The candidate central star of JAM 2 also shows indications of photometric variability, potentially due to spots on the stellar surface.

Springer Link (Chiba Institute of Technology)
Openalex Percentile: Top 5%
Stellar, planetary, and galactic studies
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