English (United Kingdom)

https://curated-unify.zendy.io/wp-json/zendy-region/v1/featured_content/oa?rat=en

https://curated-unify.zendy.io/wp-json/zendy-region/v1/highlighted_journal/

Global: Zendy Plus annual

Presents the access of premium content as premium feature

Premium Content

Presents the keyphrase highlighting as premium feature

Keyphrase Highlighting

Presents the summarisation as premium feature

Summarisation

Insights

Presents the pdf analysis as premium feature

PDF Analysis

Presents the zaia usage as premium feature

ZAIA

Global: Zendy Tools annual

Global: Zendy Free Plan

Global: Zendy Tools monthly

Global: Zendy Plus monthly

We present compelling observational evidence of G133.50+9.01 being a bonafide cloud-cloud collision candidate with signatures of induced filament, core,and cluster formation. The CO molecular line observations reveal that theG133.50+9.01 complex is made of two colliding molecular clouds with systemicvelocities, -16.9 km s-1 and -14.1 km s-1. The intersection of the clouds ischaracterised by broad bridging features characteristic of collision. Themorphology of the shocked layer at the interaction front resembles an arc likestructure with enhanced excitation temperature and H2 column density. A complexnetwork of filaments is detected in the SCUBA 850 {\mu}m image with 14 embeddeddense cores, all well correlated spatially with the shocked layer. A stellarcluster revealed through an over-density of identified Class I and II youngstellar objects is found located along the arc in the intersection regioncorroborating with a likely collision induced origin.

G133.50+9.01: A likely cloud-cloud collision complex triggering the formation of filaments, cores and a stellar cluster