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Origin of the IRAS Vela Shell: New Insights from 3D Dust Mapping

  • Authors: Bore Annie Gao, 般若 高, Catherine Zucker, Tirupati Kumara Sridharan, Cameren Swiggum, Shmuel Bialy, Theo J. O'Neill, J. E. G. Peek, Luciana Bianchi, Robert Benjamin, Lewis McCallum, Alyssa Goodman, João Alves, Charles Lada, Gordian Edenhofer, Rowan Smith, Elizabeth Watkins, Kenneth Wood, Doni Anderson

Bore Annie Gao et al 2025 The Astrophysical Journal 987 .

  • Provider: AAS Journals

Caption: Figure 4.

Probability density distributions of the IVS properties based on our fiducial model. Top panels from left to right: the inner boundary radii distribution from the geometric center; the outer boundary radii distribution from the geometric center; shell thickness. Bottom panels from left to right: peak radii distribution from the geometric center; the distribution of nH values at each peak location; distance from the Sun of the peak radii distribution.

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