Why Are (Almost) All the Protostellar Outflows Aligned in Serpens Main?
We present deep 1.4–4.8 μ m JWST-NIRCam imaging of the Serpens Main star-forming region and identify 20 candidate protostellar outflows, most with bipolar structure and identified driving sources. The outflow position angles (PAs) are strongly correlated,
Joel D. Green +6 more
doaj +1 more source
Spiers Memorial Lecture: Astrochemistry at high resolution.
Ceccarelli C.
europepmc +1 more source
Formation and Evolution of Disks Around Young Stellar Objects. [PDF]
Zhao B +11 more
europepmc +1 more source
CO IN PROTOSTARS (COPS): HERSCHEL-SPIRE SPECTROSCOPY OF EMBEDDED PROTOSTARS [PDF]
Yao-Lun Yang, Neal Evans II, Joel Green
openaire +1 more source
Mid-infrared Variability and Accretion in NGC 2264 Protostars [PDF]
S. Terebey +3 more
openalex +1 more source
Resolving the Binary Components of the Outbursting Protostar HBC 494 with ALMA [PDF]
Pedro H. Nogueira +17 more
openalex +1 more source
FIRST MAGNETIC FIELD DETECTION ON A CLASS I PROTOSTAR [PDF]
Christopher M. Johns-Krull +3 more
openalex +1 more source
Comparing star formation models with interferometric observations of the protostar NGC 1333 IRAS 4A [PDF]
P. Frau, D. Galli, J. M. Girart
openalex +1 more source
The ALMA-PILS survey: first detection of methyl isocyanide (CH3NC) in a solar-type protostar [PDF]
H. Calcutt +11 more
openalex +1 more source
Laboratory Infrared Spectra and Band Strengths of Carbonyl Sulfide (OCS) in CH<sub>3</sub>OH- and CO-Rich Ice Mixtures for Analyzing Interstellar Ice Observations. [PDF]
Slavicinska K +5 more
europepmc +1 more source

