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Cited by 47Stellar, planetary, and galactic studiesAstrophysics and Star Formation StudiesAstronomy and Astrophysical Research

Supersaturation and activity-rotation relation in PMS stars: the young cluster h Persei

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Argiroffi, C., Caramazza, M., Micela, G., Sciortino, S., Moraux, E., Bouvier, J., Flaccomio, E.·2016·Astronomy & Astrophysics
DOI 10.1051/0004-6361/201526539
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Abstract

Context. Several studies showed that the magnetic activity of late-type main-sequence (MS) stars is characterized by different regimes and that their activity levels are well described by the Rossby number, Ro, defined as the ratio between the rotational period Prot and the convective turnover time. Very young pre-main-sequence (PMS) stars show, similarly to MS stars, intense magnetic activity. However, they do not show clear activity-rotation trends, and it still debated which stellar parameters determine their magnetic activity levels.

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  • Lower activity levels for slowly rotating stars can already be seen in the 12 million year old stellar cluster h Per.

    “Such lower activity levels for slowly rotating stars can already be seen in the 12 million year old stellar cluster h Per (Argiroffi et al. 2016).”

    From The young Sun's XUV-activity as a constraint for lower CO2-limits in the Earth's Archean atmosphere (2021) · cites this paper as Argiroffi et al. 2016

    Section 5.1 says some of the slowest rotators have slightly lower X-ray luminosity, supporting the activity trend. The paper describes h Per as approximately 13 million years old, not 12 million, and limits the lower-activity finding to some stars rather than slow rotators generally. (LLM, conf=0.86)

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Cited by

Sorted by citations

Authors
Argiroffi, C., Caramazza, M., Micela, G., Sciortino, S., Moraux, E., Bouvier, J., & Flaccomio, E.
Affiliations
  • Osservatorio Astronomico di Palermo (IT)
  • Centre National de la Recherche Scientifique (FR)
ORCID
Venue
Astronomy & Astrophysics
Publisher
EDP Sciences
Published
2016-04-21
Volume
589
Pages
A113
ISSN
  • 0004-6361 (ISSN-L)
  • 1432-0746
DOI
10.1051/0004-6361/201526539
OpenAlex
W2341929365
Cited by
47
References
54
Citations by year
2026: 4 · 2025: 6 · 2024: 4 · 2023: 4 · 2022: 5 · 2021: 3 · 2020: 6 · 2019: 5 · 2018: 3 · 2017: 5 · 2016: 2
FWCI
2.39
Type
journal article
Language
en
Open access
Locations
  • Astronomy and Astrophysics (publishedVersion)
  • arXiv (Cornell University) (submittedVersion)
  • Nova Science Publishers (Nova Science Publishers, Inc.) (submittedVersion)
  • HAL (submittedVersion, other-oa)
Topics
  • Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Stellar, planetary, and galactic studies
  • Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Astrophysics and Star Formation Studies
  • Physical Sciences › Physics and Astronomy › Instrumentation › Astronomy and Astrophysical Research
Keywords
pre-main-sequence stars, stellar magnetic activity, supersaturation, rotation-activity relation, Rossby number, rotation period, convective turnover time, young stellar clusters, late-type stars

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