The inside-out planetary nebula around a born-again star View Full Text


Ontology type: schema:ScholarlyArticle      Open Access: True


Article Info

DATE

2018-10

AUTHORS

Martín A. Guerrero, Xuan Fang, Marcelo M. Miller Bertolami, Gerardo Ramos-Larios, Helge Todt, Alexandre Alarie, Laurence Sabin, Luis F. Miranda, Christophe Morisset, Carolina Kehrig, Saúl A. Zavala

ABSTRACT

Planetary nebulae are ionized clouds of gas formed by the hydrogen-rich envelopes of low- and intermediate-mass stars ejected at late evolutionary stages. The strong UV flux from their central stars causes a highly stratified ionization structure, with species of higher ionization potential closer to the star. Here, we report on the exceptional case of HuBi 1, a double-shell planetary nebula whose inner shell presents emission from low-ionization species close to the star and emission from high-ionization species farther away. Spectral analysis demonstrates that the inner shell of HuBi 1 is excited by shocks, whereas its outer shell is recombining. The anomalous excitation of these shells can be traced to its low-temperature [WC10] central star whose optical brightness has declined continuously by 10 magnitudes in a period of 46 years. Evolutionary models reveal that this star is the descendant of a low-mass star (≃1.1 M⊙) that has experienced a ‘born-again’ event1 whose ejecta shock-excite the inner shell. HuBi 1 represents the missing link in the formation of metal-rich central stars of planetary nebulae from low-mass progenitors, offering unique insight regarding the future evolution of the born-again Sakurai’s object2. Coming from a solar-mass progenitor, HuBi 1 represents a potential end-state for our Sun. Double-shell planetary nebula HuBi 1 has an inner shell that emits in low ionization potential species, and an outer shell that emits in high-ionization species. This is the inverse of the usual case. The cause is the nebula’s rapidly fading central star that went through a ‘born-again’ event. More... »

PAGES

784-789

References to SciGraph publications

Identifiers

URI

http://scigraph.springernature.com/pub.10.1038/s41550-018-0551-8

DOI

http://dx.doi.org/10.1038/s41550-018-0551-8

DIMENSIONS

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33 schema:description Planetary nebulae are ionized clouds of gas formed by the hydrogen-rich envelopes of low- and intermediate-mass stars ejected at late evolutionary stages. The strong UV flux from their central stars causes a highly stratified ionization structure, with species of higher ionization potential closer to the star. Here, we report on the exceptional case of HuBi 1, a double-shell planetary nebula whose inner shell presents emission from low-ionization species close to the star and emission from high-ionization species farther away. Spectral analysis demonstrates that the inner shell of HuBi 1 is excited by shocks, whereas its outer shell is recombining. The anomalous excitation of these shells can be traced to its low-temperature [WC10] central star whose optical brightness has declined continuously by 10 magnitudes in a period of 46 years. Evolutionary models reveal that this star is the descendant of a low-mass star (≃1.1 M⊙) that has experienced a ‘born-again’ event1 whose ejecta shock-excite the inner shell. HuBi 1 represents the missing link in the formation of metal-rich central stars of planetary nebulae from low-mass progenitors, offering unique insight regarding the future evolution of the born-again Sakurai’s object2. Coming from a solar-mass progenitor, HuBi 1 represents a potential end-state for our Sun. Double-shell planetary nebula HuBi 1 has an inner shell that emits in low ionization potential species, and an outer shell that emits in high-ionization species. This is the inverse of the usual case. The cause is the nebula’s rapidly fading central star that went through a ‘born-again’ event.
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