A planetesimal orbiting within the debris disc around a white dwarf star
(2019) In Science 364(6435). p.66-69- Abstract
Many white dwarf stars show signs of having accreted smaller bodies, implying that they may host planetary systems. A small number of these systems contain gaseous debris discs, visible through emission lines. We report a stable 123.4-minute periodic variation in the strength and shape of the Ca II emission line profiles originating from the debris disc around the white dwarf SDSS J122859.93+104032.9. We interpret this short-period signal as the signature of a solid-body planetesimal held together by its internal strength.
Please use this url to cite or link to this publication:
https://lup.lub.lu.se/record/0f213c86-2f00-4e5d-8bf1-102d4b6d0dbb
- author
- organization
- publishing date
- 2019-04-05
- type
- Contribution to journal
- publication status
- published
- subject
- keywords
- Astronomy, Planetary Sciences, Astrophysics - Earth and Planetary Astrophysics, Astrophysics - Solar and Stellar Astrophysics
- in
- Science
- volume
- 364
- issue
- 6435
- pages
- 4 pages
- publisher
- American Association for the Advancement of Science (AAAS)
- external identifiers
-
- pmid:30948547
- scopus:85064315993
- ISSN
- 1095-9203
- DOI
- 10.1126/science.aat5330
- project
- A unified picture of white dwarf planetary systems
- IMPACT: Comets, asteroids and the habitability of planets
- language
- English
- LU publication?
- yes
- id
- 0f213c86-2f00-4e5d-8bf1-102d4b6d0dbb
- alternative location
- https://arxiv.org/abs/1904.02163
- date added to LUP
- 2019-04-30 10:05:20
- date last changed
- 2024-04-16 03:26:03
@article{0f213c86-2f00-4e5d-8bf1-102d4b6d0dbb, abstract = {{<p>Many white dwarf stars show signs of having accreted smaller bodies, implying that they may host planetary systems. A small number of these systems contain gaseous debris discs, visible through emission lines. We report a stable 123.4-minute periodic variation in the strength and shape of the Ca II emission line profiles originating from the debris disc around the white dwarf SDSS J122859.93+104032.9. We interpret this short-period signal as the signature of a solid-body planetesimal held together by its internal strength.</p>}}, author = {{Manser, Christopher J. and Gänsicke, Boris T. and Eggl, Siegfried and Hollands, Mark and Izquierdo, Paula and Koester, Detlev and Landstreet, John D. and Lyra, Wladimir and Marsh, Thomas R. and Meru, Farzana and Mustill, Alexander J. and Rodríguez-Gil, Pablo and Toloza, Odette and Veras, Dimitri and Wilson, David J. and Burleigh, Matthew R. and Davies, Melvyn B. and Farihi, Jay and Fusillo, Nicola Gentile and de Martino, Domitilla and Parsons, Steven G. and Quirrenbach, Andreas and Raddi, Roberto and Reffert, Sabine and Santo, Melania Del and Schreiber, Matthias R. and Silvotti, Roberto and Toonen, Silvia and Villaver, Eva and Wyatt, Mark and Xu, Siyi and Zwart, Simon Portegies}}, issn = {{1095-9203}}, keywords = {{Astronomy; Planetary Sciences; Astrophysics - Earth and Planetary Astrophysics; Astrophysics - Solar and Stellar Astrophysics}}, language = {{eng}}, month = {{04}}, number = {{6435}}, pages = {{66--69}}, publisher = {{American Association for the Advancement of Science (AAAS)}}, series = {{Science}}, title = {{A planetesimal orbiting within the debris disc around a white dwarf star}}, url = {{http://dx.doi.org/10.1126/science.aat5330}}, doi = {{10.1126/science.aat5330}}, volume = {{364}}, year = {{2019}}, }