? Pictoris: Planets and Pulsations
- Author(s)
- Konstanze Zwintz
- Abstract
The A5 dwarf star ? Pictoris has been subject of numerous studies because it addresses several questions of stellar astrophysics, like stellar evolution, circumstellar disks, planet formation and pulsations. With V = 3.86 mag, it falls within the observable magnitude range of BRITE and is a promising target for this space mission.
- Organisation(s)
- Department of Astrophysics
- Journal
- Communications in Asteroseismology
- Volume
- 152
- Pages
- 121-123
- No. of pages
- 3
- ISSN
- 1021-2043
- DOI
- https://doi.org/10.1553/cia152s121
- Publication date
- 2008
- Peer reviewed
- Yes
- Austrian Fields of Science 2012
- 103003 Astronomy
- Portal url
- https://ucrisportal.univie.ac.at/en/publications/9c466ab3-5db2-41a2-8180-7b03bc99a9b9