SIMBAD references

1998A&A...335L..85N - Astronomy and Astrophysics, volume 335, L85-88 (1998/7-3)

Formation of undermassive single white dwarfs and the influence of planets on late stellar evolution.

NELEMANS G. and TAURIS T.M.

Abstract (from CDS):

We propose a scenario to form low-mass, single, slow rotating white dwarfs from a solar-like star accompanied by a massive planet, or a brown dwarf, in a relatively close orbit (e.g. HD 89707). Such white dwarfs were recently found by Maxted & Marsh (1998, in press). When the solar-like star ascends the giant branch it captures the planet and the subsequent spiral-in phase expels the envelope of the giant leaving a low-mass helium white dwarf remnant. In case the planet evaporizes, or fills its own Roche-lobe, the outcome is a single undermassive white dwarf. The observed distribution of planetary systems supports the applicability of this scenario.

Abstract Copyright:

Journal keyword(s): stars: giant, mass-loss, planetary systems - binaries: evolution - white dwarfs: formation

Simbad objects: 8

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2019.10.17-18:34:57

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