Investigating the Nested Structure of the Outflow from the Low Luminosity Protostar IRAS 16253-2429 Using JWST and ALMA
Mayank Narang, Himanshu Tyagi, Nagayoshi Ohashi, P. Manoj et autres
Abstract Understanding the earliest stage of star and planet formation requires detailed observations to address the connection and interplay between the accretion, outflow, and disk evolution. We present results from the observations of the low luminosity ( L bol ∼ 0.2 L …
tw, in, us, nl, de, it, dk, kr, es, gb, jp, fr, sa, cl (code pays fourni par la source)
3 citations
The Astrophysical Journal