What question did this study set out to answer?

To examine the infall properties and collapse dynamics of the massive infrared dark cloud SDC335.579-0.292.

An inverted infall profile for the collapse of the massive star-forming IRDC SDC335.579-0.292

View Full Paper

Ask AI

Bookmark

Authors

This analysis reveals an inverted infall profile in a massive star-forming region, suggesting complex collapse dynamics.

To examine the infall properties and collapse dynamics of the massive infrared dark cloud SDC335.579-0.292.
Utilized spatially-resolved HCO+ J=1–0 and H13CO+ J=1–0 maps for analysis.
Compared observations with the Hill5 model and radiative transfer models.
Examined spatial variation in molecular line emission.
Best-fit infall velocity measured at −0.6 to −1.6 km s−1.
Mass infall rate calculated between a few × 10−3 and 10−2 M⊙yr−1.
Identified a minimum infall velocity at 0.7 pc, with variations at different radii.

Jinjin et al. (2026) studied this question.

View Full Paper

Ask AI

Bookmark

View Full Paper

Ask AI

Bookmark

Authors

This analysis reveals an inverted infall profile in a massive star-forming region, suggesting complex collapse dynamics.

To examine the infall properties and collapse dynamics of the massive infrared dark cloud SDC335.579-0.292.
Utilized spatially-resolved HCO+ J=1–0 and H13CO+ J=1–0 maps for analysis.
Compared observations with the Hill5 model and radiative transfer models.
Examined spatial variation in molecular line emission.
Best-fit infall velocity measured at −0.6 to −1.6 km s−1.
Mass infall rate calculated between a few × 10−3 and 10−2 M⊙yr−1.
Identified a minimum infall velocity at 0.7 pc, with variations at different radii.

Jinjin et al. (2026) studied this question.

View Full Paper

Ask AI

Bookmark