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 a multi‐wavelength study of the region towards the GM 2‐4 nebula and the nearby source IRAS 05373+2340. Our near‐infrared H 2  1–0 S(1) line observations reveal various shock‐excited features which are part of several bipolar outflows. We identify candidates for the driving sources of the outflows from a comparison of the multi‐waveband archival data sets and spectral energy distribution (SED) modelling. The SED spectral slope () for all the protostars in the field was then compared with the visual extinction map. This comparison suggests that star formation progresses from north‐east to south‐west across this region.

GM 2‐4: a signpost for low‐ and intermediate‐mass star formation ★