Search

Image Details

View Article Bookmark & Share

Choose export citation format:

Export Citation
Large resolution
Hi-Resolution Export to PDF

A JWST, ALMA, and VLA Survey of the Ophiuchus A Star-forming Region: Unveiling Hidden Dust Mass and Connecting Infrared Outflows to Their Radio Origins

  • Authors: Isaac C. Radley, John D. Ilee, Gemma Busquet, Hauyu Baobab Liu, Klaus M. Pontoppidan, Alvaro Ribas, Marc Audard, Eleonora Bianchi, Tyler L. Bourke, Claudio Codella, Audrey Coutens, Josep M. Girart, Melvin G. Hoare, Izaskun Jiménez-Serra, Doug Johnstone, Laurent Loinard, Olja Panić, Jaime E. Pineda, Linda Podio, John J. Tobin, David J. Wilner

Isaac C. Radley et al 2026 The Astronomical Journal 172 .

  • Provider: AAS Journals

Caption: Figure 7.

Dust masses derived for each object employing three methods, ordered by class and increasing SED dust mass. Filled circles show masses derived using the multiwavelength radio SED analysis described in Section 3.4.2, with errors as shown in Table 3. The remaining two methods use a singular ALMA 1.3 mm (Band 6) flux density and Equation (5) but with differing opacities. Open squares signify masses calculated using opacities derived from our dust model (κν,DSHARP), while open diamonds adopt the S. V. W. Beckwith et al. (1990) opacity power-law prescription (κν,β).

Other Images in This Article
Image in this article
Image in this article
Image in this article
Image in this article
Image in this article
Image in this article
Image in this article
Image in this article
Image in this article

Show More

Copyright and Terms & Conditions

Additional terms of reuse