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Title: The evolution of carbon-polluted white dwarfs at low effective temperatures

Abstract

Taking advantage of the Gaia Data Release 2, recent studies have revisited the evolution of carbon-polluted white dwarfs (DQs) across a large range of effective temperatures. These analyses have clearly confirmed the existence of two distinct DQ evolutionary sequences: one with normal-mass white dwarfs and one with heavily polluted and generally more massive objects. The first sequence is thought to result from the dredge-up of carbon from the core, while the second could at least partially be made of descendants of hot DQs. However, the evolution of carbon-polluted white dwarfs below 6500 K remains unexplored, mainly due to the theoretical difficulties associated with modelling their dense atmospheres. In this work, we present a detailed star-by-star analysis of cool carbon-polluted white dwarfs. Our recently improved atmosphere models allow us to obtain good fits to most objects, including very cool DQpec white dwarfs with strongly shifted C2 molecular bands. We show herein that cool carbon-polluted white dwarfs keep following the two distinct evolutionary tracks previously identified at higher temperatures. We also find that most DQ white dwarfs transform into DQpec when their photospheric densities exceed $${\approx}0.15\, {\textrm{g\,cm}}^{-3}$$. However, we identify stars for which the DQ→DQpec transition occurs at lower photospheric densities, possibly due to the presence of a strong magnetic field.

Authors:
ORCiD logo [1];  [2]
  1. Los Alamos National Laboratory, PO Box 1663, Mail Stop B265, Los Alamos, NM 87545, USA
  2. Département de Physique, Université de Montréal, Montréal, QC H3C 3J7, Canada
Publication Date:
Research Org.:
Los Alamos National Lab. (LANL), Los Alamos, NM (United States)
Sponsoring Org.:
USDOE Laboratory Directed Research and Development (LDRD) Program; National Aeronautic and Space Administration (NASA); National Science Foundation (NSF); Gordon and Betty Moore Foundation
OSTI Identifier:
1573111
Alternate Identifier(s):
OSTI ID: 1604005
Report Number(s):
LA-UR-19-29175
Journal ID: ISSN 0035-8711
Grant/Contract Number:  
89233218CNA000001; NNX08AR22G; AST-1238877
Resource Type:
Published Article
Journal Name:
Monthly Notices of the Royal Astronomical Society
Additional Journal Information:
Journal Name: Monthly Notices of the Royal Astronomical Society Journal Volume: 490 Journal Issue: 3; Journal ID: ISSN 0035-8711
Publisher:
Royal Astronomical Society
Country of Publication:
United Kingdom
Language:
English
Subject:
79 ASTRONOMY AND ASTROPHYSICS; stars: abundances; stars: evolution; white dwarfs

Citation Formats

Blouin, Simon, and Dufour, Patrick. The evolution of carbon-polluted white dwarfs at low effective temperatures. United Kingdom: N. p., 2019. Web. doi:10.1093/mnras/stz2915.
Blouin, Simon, & Dufour, Patrick. The evolution of carbon-polluted white dwarfs at low effective temperatures. United Kingdom. doi:10.1093/mnras/stz2915.
Blouin, Simon, and Dufour, Patrick. Fri . "The evolution of carbon-polluted white dwarfs at low effective temperatures". United Kingdom. doi:10.1093/mnras/stz2915.
@article{osti_1573111,
title = {The evolution of carbon-polluted white dwarfs at low effective temperatures},
author = {Blouin, Simon and Dufour, Patrick},
abstractNote = {Taking advantage of the Gaia Data Release 2, recent studies have revisited the evolution of carbon-polluted white dwarfs (DQs) across a large range of effective temperatures. These analyses have clearly confirmed the existence of two distinct DQ evolutionary sequences: one with normal-mass white dwarfs and one with heavily polluted and generally more massive objects. The first sequence is thought to result from the dredge-up of carbon from the core, while the second could at least partially be made of descendants of hot DQs. However, the evolution of carbon-polluted white dwarfs below 6500 K remains unexplored, mainly due to the theoretical difficulties associated with modelling their dense atmospheres. In this work, we present a detailed star-by-star analysis of cool carbon-polluted white dwarfs. Our recently improved atmosphere models allow us to obtain good fits to most objects, including very cool DQpec white dwarfs with strongly shifted C2 molecular bands. We show herein that cool carbon-polluted white dwarfs keep following the two distinct evolutionary tracks previously identified at higher temperatures. We also find that most DQ white dwarfs transform into DQpec when their photospheric densities exceed ${\approx}0.15\, {\textrm{g\,cm}}^{-3}$. However, we identify stars for which the DQ→DQpec transition occurs at lower photospheric densities, possibly due to the presence of a strong magnetic field.},
doi = {10.1093/mnras/stz2915},
journal = {Monthly Notices of the Royal Astronomical Society},
number = 3,
volume = 490,
place = {United Kingdom},
year = {2019},
month = {10}
}

Journal Article:
Free Publicly Available Full Text
Publisher's Version of Record
DOI: 10.1093/mnras/stz2915

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Cited by: 1 work
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