We present the detection of a secondary outflow associated with a Class I source, Ser-emb
15, in the Serpens Molecular Cloud. We reveal two pairs of molecular outflows consisting of …

We present high-resolution high-sensitivity observations of the Class 0 protostar RCrA
IRS5N as part of the Atacama Large Milimeter/submilimeter Array large program Early …

Abstract Brown Dwarfs (BDs) are crucial objects in our understanding of both star and planet
formation, as well as in our understanding of what mechanisms shape the lower end of the …

Context. Planets form in the disks surrounding young stars. The time at which the planet
formation process begins is still an open question. Annular substructures such as rings and …

Context. HCN, HNC, and their isotopologues are ubiquitous molecules that can serve as
chemical thermometers and evolutionary tracers to characterize star-forming regions …

We use arcsec (au) resolution CO (2− 1) data from the MASSES (Mass Assembly of Stellar
Systems and their Evolution with the Submillimeter Array) project to measure the projected …

Abstract We present Atacama Large Millimeter/submillimeter Array 12-m, 7-m, and Total
Power Array observations of the FU Orionis outbursting system, covering spatial scales …

Protostellar outflows and jets play a vital role in star formation as they carry away excess
angular momentum from the inner disk surface, allowing the material to be transferred …

We investigate the possibility of the growth of magnetorotational instability (MRI) in discs
around Class 0 protostars. We construct a disc model and calculate the chemical reactions …

Brown dwarfs are the bridge between low-mass stars and giant planets. One way of
shedding light on their dominant formation mechanism is to study them at the earliest stages …