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GMRT Survey of Radio Emission from Magnetic Massive Stars. I. Emission from Single Stars at Sub-GHz Frequencies

  • Authors: Ayan Biswas, Gregg A. Wade, Barnali Das, Veronique Petit, Matthew E. Shultz

Ayan Biswas et al 2026 The Astrophysical Journal Supplement Series 285 .

  • Provider: AAS Journals

Caption: Figure 1.

Histograms showing the distribution of all the magnetic hot stars observed with GMRT/uGMRT with respect to some selected parameters. The parameters shown are as follows (from top left, clockwise): effective temperature (Teff/kK), stellar radius (R*/R), stellar mass (M*/M), rotation period (Prot/day), dipolar field strength (Bd/kG), ratio of Alfvén radius and the Kepler corotation radius (RA/RK), distance (d/pc), and mass-loss rate ﹩(\dot{M}/{M}_{\odot \,}{\mathrm{yr}}^{-1}﹩). The background histogram in red represents the complete sample, while the blue colored area represents the distribution of detected stars. Details on the sample can be found in Section 2.

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