Figure 3 from A New Class of Large-amplitude Radial-mode Hot Subdwarf Pulsators

Image Details

View Article Bookmark & Share

Choose export citation format:

Export Citation

Hi-Resolution Export to PDF PPT Format

A New Class of Large-amplitude Radial-mode Hot Subdwarf Pulsators

Authors: Thomas Kupfer, Evan B. Bauer, Kevin B. Burdge, Eric C. Bellm, Lars Bildsten, Jim Fuller, JJ Hermes, Shrinivas R. Kulkarni, Thomas A. Prince, Jan van Roestel, Richard Dekany, Dmitry A. Duev, Michael Feeney, Matteo Giomi, Matthew J. Graham, Stephen Kaye, Russ R. Laher, Frank J. Masci, Michael Porter, Reed Riddle, David L. Shupe, Roger M. Smith, Maayane T. Soumagnac, Paula Szkody, and Charlotte Ward

2019 The Astrophysical Journal Letters 878 L35.

Provider: AAS Journals

Caption: Figure 3.

T_eff–﹩\mathrm{log}(g)﹩ diagram with evolutionary tracks of low-mass He-core pre-WDs as well as low-mass He-burning stars with hydrogen envelopes of 0.5, 2.0, and 4.0 × 10⁻³ M_⊙. The color coding of the tracks corresponds to the period of the fundamental radial oscillation mode. The inset shows a zoom-in around the location of high-gravity-BLAP-2 bounded by the black rectangle. Overplotted are the BLAPs and our stars color coded with the observed period, as well as the p-mode and g-mode sdB pulsators and the two known radial mode sdB pulsators: Balloon 090100001 and CS 1246.

Other Images in This Article

Copyright and Terms & Conditions