Other formats:
BibTeX
LaTeX
RIS
@article{1406896,
author = {Murphy, Simon and Paunzen, Ernst},
article_location = {Oxford},
article_number = {1},
doi = {http://dx.doi.org/10.1093/mnras/stw3141},
keywords = {accretion; accretion discs; asteroseismology; stars: chemically peculiar; circumstellar matter; stars: distances; ISM: clouds},
language = {eng},
issn = {0035-8711},
journal = {Monthly Notices of the Royal Astronomical Society},
title = {Gaia's view of the lambda Boo star puzzle},
volume = {466},
year = {2017}
}
TY - JOUR
ID - 1406896
AU - Murphy, Simon - Paunzen, Ernst
PY - 2017
TI - Gaia's view of the lambda Boo star puzzle
JF - Monthly Notices of the Royal Astronomical Society
VL - 466
IS - 1
SP - 546-555
EP - 546-555
PB - OXFORD UNIV PRESS
SN - 00358711
KW - accretion
KW - accretion discs
KW - asteroseismology
KW - stars: chemically peculiar
KW - circumstellar matter
KW - stars: distances
KW - ISM: clouds
N2 - The evolutionary status of the chemically peculiar class of. Boo stars has been intensely debated. It is now agreed that the. Boo phenomenon affects A stars of all ages, from star formation to the terminal age main sequence, but the cause of the chemical peculiarity is still a puzzle. We revisit the debate of their ages and temperatures in order to shed light on the phenomenon, using the new parallaxes in Gaia Data Release 1 with existing Hipparcos parallaxes and multicolour photometry. We find that no single formation mechanism is able to explain all the observations, and suggest that there are multiple channels producing lambda Boo spectra. The relative importance of these channels varies with age, temperature and environment.
ER -
MURPHY, Simon and Ernst PAUNZEN. Gaia's view of the lambda Boo star puzzle. \textit{Monthly Notices of the Royal Astronomical Society}. Oxford: OXFORD UNIV PRESS, vol.~466, No~1, p.~546-555. ISSN~0035-8711. doi:10.1093/mnras/stw3141. 2017.
|
