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Baryonic Masses and Properties of Gaseous Satellite Galaxies

  • Authors: Jingyao Zhu, Yasmeen Asali, Mary E. Putman, Tobias Westmeier, W. J. G. de Blok, Barbara Catinella, Nathan Deg, Bi-Qing For, Dane Kleiner, Karen Lee-Waddell, Filippo M. Maccagni, D. J. Pisano, Austin X. Shen, Kristine Spekkens, Lister Staveley-Smith

Jingyao Zhu et al 2026 The Astrophysical Journal 1009 .

  • Provider: AAS Journals

Caption: Figure 1.

Summary of the nearby H I–bearing host galaxies in this study. Data points show the distances versus halo masses of the host galaxies (Table 1), and in parentheses is the host count from the survey: WALLABY pilot (stars; T. Westmeier et al. 2022; C. Murugeshan et al. 2024), MHONGOOSE (pentagons; W. J. G. de Blok et al. 2024), and ALFALFA from J. Zhu & M. E. Putman (2023) (small circles; H I data from M. P. Haynes et al. 2018). Colors show the fractional halo coverage (Rcover/R200; see Section 3.1). We excluded three MHONGOOSE hosts with the lowest projected halo coverages (Rcover/R200 < 0.7; see the red crosses), which are intermediate-mass spirals with no gaseous satellites in their covered inner halos (NGC 625, NGC 7793, and NGC 5068).

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