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Intertwined Birth and Death: A Herbig–Haro Outflow Resolves the Distance to Vela Junior

  • Authors: Janette Suherli, Ivo R. Seitenzahl, Samar Safi-Harb, Frédéric P. A. Vogt, Wynn C. G. Ho, Parviz Ghavamian, Chuan-Jui Li, Ashley J. Ruiter, Roland M. Crocker, Arpita Roy, Ralph Sutherland

Janette Suherli et al 2026 The Astrophysical Journal Letters 997 .

  • Provider: AAS Journals

Caption: Figure 3.

Continuum-subtracted MUSE narrowband images constructed by integrating each line over the velocity range −150 to +200 km s−1. Top row: [N I]λ5200, Hα, and [N II]λ6583 line emissions. Middle row: [S II]λ6716, [Ca II]λ7324, and [Ni II]λ7378. Bottom row [Cr II]λ8125, [Fe II]λ8617, and Pa 9 λ9229. The red square in each panel marks the position of Vela Jr CCO nebula.

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