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CARMA OBSERVATIONS OF PROTOSTELLAR OUTFLOWS IN NGC 1333
(The American Astronomical Society, 2013-09-01)
We present observations of outflows in the star-forming region NGC 1333 using the Combined Array for Research
in Millimeter-Wave Astronomy (CARMA). We combined the 12CO and 13CO (1–0) CARMA mosaics with data
from the 14 ...
Triggered massive star formation associated with the bubble HII region Sh2-39 (N5)
(EDP Sciences, 2017)
Aims. We perform a multiwavelength analysis of the bubble HII region Sh2-39 (N5) and its environs with the aim of studying the physical properties of Galactic IR bubbles and exploring their impact in triggering massive ...
Resolving the Polarized Dust Emission of the Disk around the Massive Star Powering the HH 80-81 Radio Jet
(IOP Publishing, 2018-04)
Here we present deep (16 μJy beam-1), very high (40 mas) angular resolution 1.14 mm, polarimetric, Atacama Large Millimeter/submillimeter Array (ALMA) observations toward the massive protostar driving the HH 80-81 radio ...
Dust-correlated centimetre-wave radiation from the M78 reflection nebula
(2011)
An anomalous radio continuum component at cm-wavelengths has been observed in various sources, including dark clouds. This continuum component represents a new property of the ISM. In this work we focus on one particular ...
Complex AGN feedback in the Teacup galaxy: a powerful ionised galactic outflow, jet-ISM interaction, and evidence for AGN-triggered star formation in a giant bubble
(2023)
Context: The z ∼ 0.1 type-2 QSO J1430+1339, known as the “Teacup”, is a complex galaxy showing a loop of ionised gas ∼10 kpc in diameter, co-spatial radio bubbles, a compact (∼1 kpc) jet, and outflow activity. Its closeness ...
Dust-correlated centimetre-wave radiation from the M78 reflection nebula
(2011)
An anomalous radio continuum component at cm-wavelengths has been observed in various sources, including dark clouds. This continuum component represents a new property of the ISM. In this work we focus on one particular ...
Planck intermediate results. XVIII. The millimetre and sub-millimetre emission from planetary nebulae
(EDP Sciences, 2015)
Late stages of stellar evolution are characterized by copious mass-loss events whose signature is the formation of circumstellar envelopes (CSE).
Planck multi-frequency measurements have provided relevant information on ...