NSV11749, an elder sibling of the born-again stars V605Aql and V4334Sgr?
We argue that NSV11749, an eruption observed in the early twentieth century, was a rare event known as "very late thermal pulse" (VLTP). To support our argument we compare the light curve of NSV11749 with those of the two bona fide VLTP objects known to date, V4334Sgr and V605Aql, and with...
Guardado en:
Autores principales: | Miller Bertolami, Marcelo Miguel, Rohrmann, René, Granada, Anahí, Althaus, Leandro Gabriel |
---|---|
Formato: | Articulo |
Lenguaje: | Inglés |
Publicado: |
2011
|
Materias: | |
Acceso en línea: | http://sedici.unlp.edu.ar/handle/10915/84686 |
Aporte de: |
Ejemplares similares
-
The born-again (very late thermal pulse) scenario revisited: The mass of the remnants and implications for V4334 Sgr
por: Miller Bertolami, Marcelo Miguel, et al.
Publicado: (2007) -
Breaking news from the HST: the central star of the Stingray Nebula is now returning towards the AGB
por: Reindl, Nicole, et al.
Publicado: (2017) -
New evolutionary calculations for the born again scenario
por: Miller Bertolami, Marcelo Miguel, et al.
Publicado: (2006) -
Oscillatory secular modes: The thermal micropulses
por: Gautschy, A., et al.
Publicado: (2007) -
Full evolutionary models for PG 1159 stars. Implications for the helium-rich O(He) stars
por: Miller Bertolami, Marcelo Miguel, et al.
Publicado: (2006)