Magnetic Ap Stars in the Hertzsprung-Russell Diagram

By S. Hubrig, P. North, G. Mathys. 2000

143 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Instrumentation

View Paper: https://www.semanticscholar.org/paper/b0e86855e8005040732b4871dc3e068fa50ce852

How researchers see this paper

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In Astronomy and Astrophysics

1. J. Braithwaite
2. F. Royer
3. J. Zorec
4. Åke Nordlund
5. G. Bryden
6. K. Stapelfeldt
7. K. Su
8. A. Paris

In Instrumentation

1. G. Bryden
2. K. Stapelfeldt
3. F. Royer
4. Åke Nordlund
5. R. O. Gray
6. Christine Chen
7. G. Rieke
8. O. Kochukhov

Citations in the corpus

• Debris Disks in Main-Sequence Binary Systems (2006, background): “HD 137909 is part of an extensive study by Hubrig et al. (2000), who put it on the H-R diagram and find it to be well above the zero-age main sequence, implying that this system is old.”
• Evolutionary state of magnetic chemically peculiar stars (2006, methodology): “Parallaxes with an accuracy better than 20% (which is the same threshold as employed by Hubrig et al. 2000) could be retrieved for 150 magnetic CP stars.”
• Rotational velocities of A-type stars. III. Velocity distributions (2006, background): “The Ap phenomenon is, however, evolutionary related, because it appears after the stars completed at least the first third of their MS life (Hubrig et al. 2000; Stȩpień 2000).”
• Stable magnetic fields in stellar interiors (2005, background): “1.1 of Hubrig et al. (2000a), that Ap stars are typically more than 30% of the way through their main-sequence life.”
• Catalogue of Ap, HgMn and Am stars (2009, background): “…efforts have been brought into the analysis of magnetic fields (e.g., Mathys 1991, 1995; Mathys & Lanz 1992; Mathys & Hubrig 1997; Mathys et al. 1997; Hubrig et al. 2000, 2004, 2005, 2006; Aurière et al. 2007; Wade et al. 2000; and the catalogue by Bychkov et al. 2003, and references therein).”
• Rotational velocities of A-type stars - IV. Evolution of rotational velocities (2012, background): “However, the slow rotation of Am stars can be caused by tidal braking because they are known to be binaries (Debernardi 2000), while the Ap characteristics can be favored by the magnetic braking in MS evolutionary phase (Hubrig et al. 2000; Stȩpień 2000).”