Results 41 to 50 of about 1,150 (163)
EPISODE. III. The Nested Jet/Outflow Morphology of EC 53 Revealed by JWST and ALMA
We present an extensive study of the structure and kinematics of the jet and outflow of EC 53, a Class I protostar with a quasiperiodic variability, using combined James Webb Space Telescope (JWST) and Atacama Large Millimeter/submillimeter Array (ALMA ...
Seonjae Lee +10 more
doaj +1 more source
Molecular Outflows from Young Stellar Objects
30 pages, 6 figures. To appear in Protostars & Planets IV, eds. V. Mannings, A. Boss, S. Russell (Tucson: The University of Arizona Press)
Richer, John +4 more
openaire +2 more sources
Illuminating Youth: Decades of Mid-infrared Variability and Color Evolution of Young Stellar Objects
The variability of young stellar objects (YSOs) is a crucial tool for understanding the mechanisms driving flux changes. In this study, we present an infrared variability analysis of a large sample of over 20,000 candidate YSOs, using data from the ...
Sharma Neha, Saurabh Sharma
doaj +1 more source
We present images of IRAS 08235–4316 with the Dark Energy Camera Plane Survey (DECaPS; spanning 0.398–1.034 μ m, at ∼1″ resolution) and the Submillimeter Array (SMA; at 1.38 mm (217 GHz) and ∼1 $\mathop{.}\limits^{^{\prime\prime} }$ 9 × 1 $\mathop ...
Joshua Bennett Lovell +6 more
doaj +1 more source
The Structure and Kinematics of Three Class 0 Protostellar Jets from JWST
We present observations of jets within 2000 au of three deeply embedded protostars using 2.9–27 μ m observations with JWST. These observations show the morphologies and kinematics of the collimated jets from three protostars, the low-mass Class 0 ...
Samuel A. Federman +22 more
doaj +1 more source
We present the Atacama Large Millimeter/submillimeter Array Band 7 observations of the CO ( J = 3−2) line emission of the protostellar system HH 212 at ∼24 au spatial resolution and compare them to those of the SiO ( J = 8−7) and SO ( J = 8−7) line ...
J. A. López-Vázquez +10 more
doaj +1 more source
CO Outflows from Young Stellar Objects
We have mapped the CO J = 1-0 emission from molecular outflows associated with six young stellar systems using the BIMA array. The systems are all relatively nearby, have low-luminosity, and range from Class 0 to Class II sources. The CO outflows in these systems are complicated, showing multipolar structures, multiple cavities, and asymmetric lobes ...
Chin‐Fei Lee +3 more
openaire +1 more source
Multiple Shells Driven by Disk Winds: ALMA Observations in the HH 30 Outflow
We present archival Atacama Large Millimeter/submillimeter Array band 6 observations of the ^13 CO ( J = 2–1) and ^12 CO ( J = 2–1) molecular line emission of the protostellar system associated with HH 30.
J. A. López-Vázquez +5 more
doaj +1 more source
LAMOST Reveals Long-lived Protoplanetary Disks
While both observations and theories demonstrate that protoplanetary disks are not expected to live much longer than ∼10 Myr, several examples of prolonged disks have been observed in the past.
Xiao-Long Wang +4 more
doaj +1 more source
IRAS22150+6190: A POORLY STUDIED YOUNG STAR
Many young stellar objects have been discovered in the course of the InfraRed Astronomical Satellite (IRAS) mission, which observed almost the entire sky in four photometric bands between 12 and 100 microns in 1989.
K. S. Kuratov +3 more
doaj +1 more source

