A Magnetic Snapshot Survey of F-Type Stars

Author:

Seach J M1,Marsden S C1,Carter B D1,Neiner C2ORCID,Folsom C P3,Mengel M W1ORCID,Oksala M E24,Buysschaert B25

Affiliation:

1. University of Southern Queensland, Centre for Astrophysics, Toowoomba 4350, Australia

2. LESIA, Paris Observatory, PSL University, CNRS, Sorbonne University, Université de Paris, 5 place Jules Janssen, 92195 Meudon, France

3. IRAP, Université Toulouse, CNRS, CNES, UPS, F-31400 Toulouse, France

4. Department of Physics, California Lutheran University, 60 West Olsen Road # 3700, Thousand Oaks, CA 91360, USA

5. Instituut voor Sterrenkunde, KU Leuven, Celestijnenlaan 200D, 3001 Leuven, Belgium

Abstract

Abstract We present a spectropolarimetric magnetic snapshot survey of 55 stars which includes 53 F-type stars ranging from spectral types F0 to F9 plus 2 chemically peculiar stars β CrB, and δ Cap. We look for magnetic fields in stars spanning a range of effective temperatures where the transition from fossil to dynamo magnetic fields is believed to occur. High-resolution spectropolarimetry using circularly polarized spectra is used to look for a magnetic detection in the Stokes V profile, determine the mean longitudinal magnetic field (Bl), and to look for correlations with stellar parameters. Surface magnetic fields are detected on 14 F-stars, and present in every spectral class from F3V-F9V ranging in strength from 0.3 ± 0.1 G (36 UMa, F8V) to 8.3 ± 0.9 G (h Dra, F8V). Thus we find photospheric magnetic fields are present in stars as early as spectral type F3V with an outer convection zone thickness less than a few per cent of the stellar radius.

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

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