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Low-Metallicity Star Formation Survey of Sh2-284 (LZ-STAR): The Core Mass Function

  • Authors: Yu Cheng, 宇 程, Jonathan C. Tan, Morten Andersen, Alva Kinman, Rubén Fedriani, Kei E. I. Tanaka, Yichen Zhang

Yu Cheng et al 2026 The Astrophysical Journal Letters 1009 .

  • Provider: AAS Journals

Caption: Figure C1.

Observed core sizes and aspect ratios as a function of core mass. The left panel shows the observed core size, defined as the geometric mean FWHM, ﹩{\theta }_{{\rm{FWHM}}}={({\theta }_{{\rm{maj}}}{\theta }_{{\rm{\min }}})}^{1/2}﹩, without deconvolving the ALMA synthesized beam. The red curve shows the empirical size model adopted for the core insertion experiments, obtained from a robust linear regression: ﹩{\mathrm{log}}_{10}({\theta }_{\mathrm{FWHM}}\,{\mathrm{arcsec}}^{-1})=-0.135+0.150\,{\mathrm{log}}_{10}(M/{M}_{\odot })﹩. The shaded region shows the 1σ scatter, estimated as the standard deviation of the residuals in ﹩{\mathrm{log}}_{10}{\theta }_{{\rm{FWHM}}}﹩ around this relation. The trend is held fixed above 10 M⊙ since only a few cores are available. The right panel shows the observed aspect ratio, ﹩{\theta }_{{\rm{maj}}}/{\theta }_{{\rm{\min }}}﹩. The upper axis gives the corresponding 1.3 mm flux density.

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