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Discovery of a Compact Companion to the Hot Subdwarf Star BD +37° 442

  • Authors: Nicola La Palombara, Sandro Mereghetti, Andrea Tiengo, and Paolo Esposito

La Palombara et al. 2012 The Astrophysical Journal Letters 750 L34.

  • Provider: AAS Journals

Caption: Figure 4.

Estimated wind-accretion X-ray luminosity of BD +37° 442 as a function of the binary period, in the case of a WD (dashed lines) and an NS (solid lines). The couples of lines refer to two values of the wind velocity index β = 0.6 and β = 1. The horizontal dotted lines represent the minimum and maximum of the estimated luminosity of the blackbody component.

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