Hostname: page-component-cd9895bd7-hc48f Total loading time: 0 Render date: 2024-12-25T16:21:07.844Z Has data issue: false hasContentIssue false
  • English
  • Français

The completeness of Gaia-selected samples of white dwarfs

Published online by Cambridge University Press:  09 October 2020

Terry D. Oswalt Open the ORCID record for Terry D. Oswalt [Opens in a new window] ,
Jay B. Holberg  and
Edward M. Sion
Terry D. Oswalt
Affiliation:
Department of Physical Sciences, Embry-Riddle Aeronautical University, 1 Aerospace Blvd., Daytona Beach, FL32114USA email: [email protected]
Jay B. Holberg
Affiliation:
Lunar & Planetary Laboratory, University of Arizona, Tucson, AZ75201USA email: [email protected]
Edward M. Sion
Affiliation:
Department of Astronomy & Astrophysics, Villanova UniversityVillanova, PA19085USA email: [email protected]
Rights & Permissions [Opens in a new window]

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

The Gaia DR2 has dramatically increased the ability to detect faint nearby white dwarfs. The census of the local white dwarf population has recently been extended from 25 pc to 50 pc, effectively increasing the sample by roughly an order of magnitude. Here we examine the completeness of this new sample as a function of variables such as apparent magnitude, distance, proper motion, photometric color index, unresolved components, etc.

Keywords

starswhite dwarfsGaia
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 15 , Symposium S357: White Dwarfs as Probes of Fundamental Physics: Tracers of Planetary, Stellar and Galactic Evolution , October 2019 , pp. 170 - 174
Copyright
© International Astronomical Union 2020

References

Fontaine, G., Brassard, P., & Bergeron, P. 2001, PASP, 113, 409CrossRefGoogle Scholar
Gaia, Collaboration 2016, A&A 616, A1Google Scholar
Garcia-Berro, E. & Oswalt, T.D. 2016, New Astron. Rev. 72, 1CrossRefGoogle Scholar
Gentile Fusillo, N., Tremblay, P.-E., Gansicke, B., Manser, C., Cunningham, T., Cukanovaite, E., Hollands, M., Marsh, T., Raddi, R., Jordan, S., Toonen, S., Geier, S., Barstow, M., Cummings, J., et al. 2019, MNRAS, 482, 4570CrossRefGoogle Scholar
Harris, H. C., Munn, J. A., Kilic, M., Liebert, J., Williams, K. A., von Hippel, T., Levine, S. E., Monet, D. G., Eisenstein, D. J., Kleinman, S. J., Metcalfe, T. S., Nitta, A., Winget, D. E., Brinkmann, J., Fukugita, M., Knapp, G. R., Lupton, R. H., Smith, J. A., Schneider, D. P., et al. 2006, AJ, 131, 571CrossRefGoogle Scholar
Holberg, J. B., Oswalt, T. D., Sion, E. M., McCook, G. P., et al. 2016, MNRAS 462, 2295CrossRefGoogle Scholar
Jimenez-Esteban, F., Torres, S., Rebassa-Mansergas, A., Skorobogatov, G., Solano, E., Cantero, C., Rodrigo, C., et al. 2018, MNRAS 480, 4505CrossRefGoogle Scholar
Kepler, S., Pelisoli, I., Jordan, S., Kleinman, S., Koester, D., Kulebi, B., Pecanha, V., Castanheira, B., Nitta, A., Costa, J., Winget, D., Kanaan, A., Fraga, L., et al. 2013, MNRAS 429 2934CrossRefGoogle Scholar
Oswalt, T., Holberg, J., & Sion, E. 2017, ASPC 509, 59Google Scholar
Rebassa-Mansergas, A., Toonen, S., Torres, S., Canals, P., et al. 2019, MNRAS, (in press), astro-ph 1911.13128v1Google Scholar
Torres, S., Cantero, C., Rebassa-Mansergas, A., Skorobogatov, G., Jimenez-Esteban, F., Solano, S., et al. 2019, MNRAS 485, 5573CrossRefGoogle Scholar
Tremblay, P.-E., Fontaine, G., Gentile Fusillo, N., Dunlap, B., Gansicke, B., Hollands, M., Hermes, J., Marsh, T., Cukanovaite, E., Cunningham, T., et al. 2019, Nature, L565, 202CrossRefGoogle Scholar