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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 10.

The number of H I–bearing satellite candidates versus host stellar mass for hosts in interacting pairs (“int”) or with MC-like massive satellites. Matching symbols identify each primary–secondary system; the lower-mass point counts the satellites associated with the secondary. More isolated hosts (small circles) and the binned statistics of the full sample are shown for comparison (as in Figure 9; host M*–M200 conversions are listed in Table 1).

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