Stellar Archaeology with Gaia: The Galactic White Dwarf Population

B. Gänsicke; P. Tremblay; M. Barstow; G. Bono; M. Burleigh; S. Casewell; V. Dhillon; J. Farihi; E. Garcia-Berro; S. Geier; N. Gentile-Fusillo; J. Hermes; M. Hollands; A. Istrate; S. Jordan; C. Knigge; C. Manser; T. Marsh; G. Nelemans; A. Pala; R. Raddi; T. Tauris; O. Toloza; D. Veras; K. Werner; D. Wilson

Stellar Archaeology with Gaia: The Galactic White Dwarf Population

B. Gänsicke, P. Tremblay, M. Barstow, G. Bono, M. Burleigh, S. Casewell, V. Dhillon, J. Farihi, E. Garcia-Berro, S. Geier, N. Gentile-Fusillo, J. Hermes, M. Hollands, A. Istrate, S. Jordan, C. Knigge, C. Manser, T. Marsh, G. Nelemans, A. PalaR. Raddi, T. Tauris, O. Toloza, D. Veras, K. Werner, D. Wilson

Research output: Contribution to book/anthology/report/conference proceeding › Book chapter › Research

Abstract

Gaia will identify several 10⁵ white dwarfs, most of which will be in the solar neighborhood at distances of a few hundred parsecs. Ground-based optical follow-up spectroscopy of this sample of stellar remnants is essential to unlock the enormous scientific potential it holds for our understanding of stellar evolution, and the Galactic formation history of both stars and planets.

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Original language	Undefined/Unknown
Title of host publication	Multi-Object Spectroscopy in the Next Decade: Big Questions, Large Surveys, and Wide Fields
Publication date	Oct 2016
Publication status	Published - Oct 2016

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Gänsicke, B., Tremblay, P., Barstow, M., Bono, G., Burleigh, M., Casewell, S., Dhillon, V., Farihi, J., Garcia-Berro, E., Geier, S., Gentile-Fusillo, N., Hermes, J., Hollands, M., Istrate, A., Jordan, S., Knigge, C., Manser, C., Marsh, T., Nelemans, G., ... Wilson, D. (2016). Stellar Archaeology with Gaia: The Galactic White Dwarf Population. In Multi-Object Spectroscopy in the Next Decade: Big Questions, Large Surveys, and Wide Fields

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title = "Stellar Archaeology with Gaia: The Galactic White Dwarf Population",

abstract = "Gaia will identify several 105 white dwarfs, most of which will be in the solar neighborhood at distances of a few hundred parsecs. Ground-based optical follow-up spectroscopy of this sample of stellar remnants is essential to unlock the enormous scientific potential it holds for our understanding of stellar evolution, and the Galactic formation history of both stars and planets. ...",

author = "B. G{\"a}nsicke and P. Tremblay and M. Barstow and G. Bono and M. Burleigh and S. Casewell and V. Dhillon and J. Farihi and E. Garcia-Berro and S. Geier and N. Gentile-Fusillo and J. Hermes and M. Hollands and A. Istrate and S. Jordan and C. Knigge and C. Manser and T. Marsh and G. Nelemans and A. Pala and R. Raddi and T. Tauris and O. Toloza and D. Veras and K. Werner and D. Wilson",

year = "2016",

month = oct,

language = "Udefineret/Ukendt",

booktitle = "Multi-Object Spectroscopy in the Next Decade: Big Questions, Large Surveys, and Wide Fields",

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Gänsicke, B, Tremblay, P, Barstow, M, Bono, G, Burleigh, M, Casewell, S, Dhillon, V, Farihi, J, Garcia-Berro, E, Geier, S, Gentile-Fusillo, N, Hermes, J, Hollands, M, Istrate, A, Jordan, S, Knigge, C, Manser, C, Marsh, T, Nelemans, G, Pala, A, Raddi, R, Tauris, T, Toloza, O, Veras, D, Werner, K & Wilson, D 2016, Stellar Archaeology with Gaia: The Galactic White Dwarf Population. in Multi-Object Spectroscopy in the Next Decade: Big Questions, Large Surveys, and Wide Fields.

TY - CHAP

T1 - Stellar Archaeology with Gaia: The Galactic White Dwarf Population

AU - Gänsicke, B.

AU - Tremblay, P.

AU - Barstow, M.

AU - Bono, G.

AU - Burleigh, M.

AU - Casewell, S.

AU - Dhillon, V.

AU - Farihi, J.

AU - Garcia-Berro, E.

AU - Geier, S.

AU - Gentile-Fusillo, N.

AU - Hermes, J.

AU - Hollands, M.

AU - Istrate, A.

AU - Jordan, S.

AU - Knigge, C.

AU - Manser, C.

AU - Marsh, T.

AU - Nelemans, G.

AU - Pala, A.

AU - Raddi, R.

AU - Tauris, T.

AU - Toloza, O.

AU - Veras, D.

AU - Werner, K.

AU - Wilson, D.

PY - 2016/10

Y1 - 2016/10

N2 - Gaia will identify several 105 white dwarfs, most of which will be in the solar neighborhood at distances of a few hundred parsecs. Ground-based optical follow-up spectroscopy of this sample of stellar remnants is essential to unlock the enormous scientific potential it holds for our understanding of stellar evolution, and the Galactic formation history of both stars and planets. ...

AB - Gaia will identify several 105 white dwarfs, most of which will be in the solar neighborhood at distances of a few hundred parsecs. Ground-based optical follow-up spectroscopy of this sample of stellar remnants is essential to unlock the enormous scientific potential it holds for our understanding of stellar evolution, and the Galactic formation history of both stars and planets. ...

M3 - Bidrag til bog/antologi

BT - Multi-Object Spectroscopy in the Next Decade: Big Questions, Large Surveys, and Wide Fields

ER -