Nonradiative Activity across the H-R Diagram - which Types of Stars are Solar-Like
Abstract
Major advances in our understanding of nonradiatively heated outer atmospheric layers (coronae, transition regions, and chromospheres) and other solar-like activity in stars has occurred in the past few years primarily as a result of ultraviolet spectroscopy from IUE, X-ray imaging from the Einstein Observatory, microwave detections by the VLA, and new optical observing techniques. I critically review the observational evidence and comment upon the trends with spectral type, gravity, age, and rotational velocity that are now becoming apparent. I define a solar-like star as one which has a turbulent magnetic field sufficiently strong to control the dynamics and energetics in its outer atmospheric regions. The best indicator of a solar-like star is the direct measurement of a strong, variable magnetic field and such data are now becoming available, but good indirect indicators include photometric variability on a rotational time scale indicating dark starspots and nonthermal microwave emission. X-rays and ultraviolet emission lines produced by plasma hotter than 104 K imply nonradiative heating processes that are likely magnetic in character, except for the hot stars where the heating is likely by shocks in the wind resulting from radiative instabilities. I conclude that dwarf stars of spectral type G-M and rapidly rotating subgiants and giants of spectral type F-K in spectroscopic binary systems are definitely solar-like. Dwarf stars of spectral type A7-F7 are almost certainly solar-like, and T Tauri and other pre-Main-Sequence stars are probably solar-like. Slowly rotating single giants of spectral type F to early K are also probably solar-like, and the helium-strong hottest Bp stars are interesting candidates for being solar-like. The O and B stars exhibit some aspects of activity but probably have weak fields and are not solar-like. Finally, the A dwarfs and the cool giants and supergiants show no evidence of being solar-like.
- Publication:
-
Solar Physics
- Pub Date:
- October 1985
- DOI:
- 10.1007/BF00158435
- Bibcode:
- 1985SoPh..100..333L
- Keywords:
-
- Astrophysics;
- Hertzsprung-Russell Diagram;
- Stellar Activity;
- Dwarf Stars;
- Giant Stars;
- Pre-Main Sequence Stars;
- Stellar Magnetic Fields;
- Subgiant Stars;
- T Tauri Stars;
- X Ray Astronomy;
- Astrophysics;
- Spectral Type;
- Variable Magnetic Field;
- Microwave Emission;
- Dwarf Star;
- Photometric Variability