K 1-6 is a photoionised ISM nebula shaped by a fast-moving hot white dwarf in a triple system

arXiv:2607.12850 · astro-ph.SR · Submitted 2026-07-14 · Read on arXiv

Jaroslav Merc, David Jones, Ana Escorza, Henri M. J. Boffin, Nicole Reindl, Michael Abdul-Masih, Thomas Masseron, Paulina Sowicka, Jan Kára, Jorge García-Rojas, Rafael A. García, Dinil B. Palakkatharappil, Quentin A. Parker, Albert A. Zijlstra, Diego Godoy-Rivera, Paul G. Beck, Savita Mathur, Montserrat Armas Padilla, Teo Muñoz Darias, Hana Kučáková, Marek Wolf, Kamil Hornoch, Petr Zasche, Rosa Clavero, Peter Goodhew

astro-ph.SR

Submitted: 2026-07-14

Comments: 13 pages, 13 figures + appendices; accepted in A&A

License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/

Terminology

Abundance — 9× in this paper · explained in 1 episode
Hubble Space Telescope — 5× in this paper
Core — 4× in this paper · explained in 2 episodes
Telescopio Nazionale Galileo — 4× in this paper
Active Regions — 2× in this paper · explained in 1 episode
Adam — 2× in this paper · explained in 2 episodes
Aperture — 2× in this paper · explained in 1 episode
Gran Telescopio Canarias — 2× in this paper
Northern Sky Variability Survey — 2× in this paper
Trace — 2× in this paper · explained in 2 episodes
Alignment — 1× in this paper · explained in 1 episode
Aperture Photometry — 1× in this paper · explained in 1 episode
Consistency — 1× in this paper · explained in 3 episodes
Cosmic Origins Spectrograph — 1× in this paper
Metallicity — 1× in this paper · explained in 3 episodes
Renormalised Unit Weight Error — 1× in this paper

Sources

Thermally inflated accretors in post-mass transfer binaries: Abell 35 and its class revisited

Terminology

Sources

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