Results 141 to 150 of about 25,326 (243)
Effects of turbulence and rotation on protostar formation as a precursor of massive black holes [PDF]
C. Van Borm +5 more
openalex +1 more source
Dust Polarization toward Embedded Protostars in Ophiuchus with ALMA. I. VLA 1623 [PDF]
Sarah I. Sadavoy +9 more
openalex +1 more source
We present Atacama Large Millimeter/submillimeter Array (ALMA) observations of the Class 0 protostar IRAS 04166+2706, obtained as part of the ALMA Large Program Early Planet Formation in Embedded Disks.
Nguyen Thi Phuong +22 more
doaj +1 more source
Mid-infrared Variability and Accretion in NGC 2264 Protostars [PDF]
S. Terebey +3 more
openalex +1 more source
L1448 IRS3B: Dust Polarization Aligned with Spiral Features, Tracing Gas Flows
Circumstellar disk dust polarization in the (sub)millimeter is, for the most part, not from dust grain alignment with magnetic fields but rather indicative of a combination of dust self-scattering with a yet unknown alignment mechanism that is consistent
Leslie W. Looney +13 more
doaj +1 more source
Multiple Jets in the Bursting Protostar HOPS 373SW
We present the outflows detected in HOPS 373SW, a protostar undergoing a modest 30% brightness increase at 850 μ m. Atacama Large Millimeter/submillimeter Array observations of shock tracers, including SiO 8–7, CH _3 OH 7 _k –6 _k , and ^12 CO 3–2 ...
Seokho Lee +4 more
doaj +1 more source
Ionisation And The Formation Of Low-Mass Protostars
James Wurster +2 more
openalex +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
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

