A connection between the morphology of the X-ray emission and rotation for solar-type stars in open clusters

Abstract

It is suggested that the three-segmented morphology of the soft X-ray emission from cluster and field stars may be understood in terms of the recent classification of rotating stars into three kinds: those lying on the convective sequence, on the interface sequence, or in the gap between them.

7 pages, 1 (color) figure, accepted by ApJ Letters

References in corpus (1)

• On the rotational evolution of solar- and late-type stars, its magnetic origins, and the possibility of stellar gyrochronology

Cited by in corpus (33)

• The stellar activity-rotation relationship and the evolution of stellar dynamos
• Ages for illustrative field stars using gyrochronology: viability, limitations and errors
• The Origin of T Tauri X-ray Emission: New Insights from the Chandra Orion Ultradeep Project
• The Habitability of Planets Orbiting M-dwarf Stars
• The evolution of X-ray emission in young stars
• Rotational velocities of A-type stars IV. Evolution of rotational velocities
• Rotational velocities of A-type stars. III. Velocity distributions
• Magnetic Braking Formulation for Sun-Like Stars: Dependence on Dipole Field Strength and Rotation Rate
• Dynamical Mass of the Substellar Benchmark Binary HD 130948BC
• The flare catalog and the flare activity in the Kepler mission
• X-ray Properties of Pre--Main-Sequence Stars in the Orion Nebula Cluster with Known Rotation Periods
• Stellar activity with LAMOST - II. Chromospheric activity in open clusters
• Stellar Activity and Coronal Heating: an overview of recent results
• Rotation and activity of pre-main-sequence stars
• Stellar Rotation in the Gaia Era: Revised Open Clusters Sequences
• A 4 Gyr M-dwarf Gyrochrone from CFHT/MegaPrime Monitoring of the Open Cluster M67
• M dwarf companions to white dwarfs I: relating magnetic activity, rotation and age
• A method to estimate stellar ages from kinematical data
• The rotation period distribution of the rich Pleiades-age Southern open cluster NGC 2516. Existence of a representative zero-age main sequence distribution
• Signature of Planetary Mergers on Stellar Spins
• Long-term monitoring in IC4665: Fast rotation and weak variability in very low mass objects
• Testing the Limits of Precise Subgiant Characterization with APOGEE and Gaia: Opening a Window to Unprecedented Astrophysical Studies
• The Factory and the Beehive. IV. A Comprehensive Study of the Rotation X-ray Activity Relation in Praesepe and the Hyades
• High-energy spectra of LTT 1445A and GJ 486 reveal flares and activity
• Kepler main-sequence solar-like stars: surface rotation and magnetic-activity evolution
• Flare Activity of Wide Binary Stars with Kepler
• FK Comae Berenices, King of Spin: The COCOA-PUFS Project
• Temporal changes of the flare activity of Proxima Cen
• The Role of White Dwarfs in Cataclysmic Variable Spin-down
• Coronal Temperature as an Age Indicator
• Four ages of rotating stars in the rotation--activity relationship and gyrochronology
• Chromospheric Activity in 55 Cancri: II. Theoretical Wave Studies versus Observations
• Asymmetric emissions of neutrinos in the cooling of rotating proto-neutron stars