An explanation for the double birth cry of a newborn star
An article published in the journal “The Astrophysical Journal” reports the analysis that led to unveil the origin of two gas flows from the newborn star MMS5/OMC-3. A team of researchers used the ALMA radio telescope to study this situation which was a mystery because there are two very different flows since one is a slow outflow while the other is a fast jet and they concluded that they were formed independently in different parts of the gas disk surrounding the star.




