Wide field CO J =3 → 2 mapping of the Serpens cloud core

@article{Dionatos2010WideFC,
  title={Wide field CO J =3 → 2 mapping of the Serpens cloud core},
  author={Odysseas Dionatos and Brunella Nisini and Claudio Codella and Teresa Giannini},
  journal={Astronomy and Astrophysics},
  year={2010},
  volume={523}
}
Context. Outflows provide indirect means to gain insight into diverse star formation-associated phenomena. At the level of individual protostellar cores, both outflows and the intrinsic core properties can be used to study the mass accretion/ejection process of heavily embedded protostellar sources. Aims. The main objective of the paper is to study the overall outflow distribution and its association with the young population of the Serpens Core cluster. In addition, the paper addresses the… 
Feedback of atomic jets from embedded protostars in NGC 1333
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Chemical and kinematic structure of extremely high-velocity molecular jets in the Serpens Main star-forming region
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Context. Water is a key tracer of dynamics and chemistry in low-mass star-forming regions, but spectrally resolved observations have so far been limited in sensitivity and angular resolution, and
Atomic jet from SMM1 (FIRS1) in Serpens uncovers protobinary companion
We report on the detection of an atomic jet associated with the protostellar source SMM1 (FIRS1) in Serpens. The jet is revealed in [FeII] and [NeII] line maps observed with Spitzer/IRS, and further
The Circumstellar Environment around the Embedded Protostar EC 53
EC53 is an embedded protostar with quasi-periodic emission in the near-IR and sub-mm. We use ALMA high-resolution observations of continuum and molecular line emission to describe the circumstellar
The JCMT Transient Survey: Detection of sub-mm variability in a Class I protostar EC 53 in Serpens Main
During the protostellar phase of stellar evolution, accretion onto the star is expected to be variable, but this suspected variability has been difficult to detect because protostars are deeply
Investigating Particle Acceleration in Protostellar Jets: The Triple Radio Continuum Source in Serpens
While most protostellar jets present free-free emission at radio wavelengths, synchrotron emission has been also proposed to be present in a handful of these objects. The presence of non-thermal
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