Astrochemistry during the formation of stars
JK Jørgensen, A Belloche… - Annual Review of …, 2020 - annualreviews.org
Star-forming regions show a rich and varied chemistry, including the presence of complex
organic molecules—in both the cold gas distributed on large scales and the hot regions …
organic molecules—in both the cold gas distributed on large scales and the hot regions …
Protostellar outflows
J Bally - Annual Review of Astronomy and Astrophysics, 2016 - annualreviews.org
Outflows from accreting, rotating, and magnetized systems are ubiquitous. Protostellar
outflows can be observed from radio to X-ray wavelengths in the continuum and a multitude …
outflows can be observed from radio to X-ray wavelengths in the continuum and a multitude …
TADPOL: A 1.3 mm survey of dust polarization in star-forming cores and regions
We present λ 1.3 mm Combined Array for Research in Millimeter-wave Astronomy
observations of dust polarization toward 30 star-forming cores and eight star-forming regions …
observations of dust polarization toward 30 star-forming cores and eight star-forming regions …
Herschel observations of extraordinary sources: analysis of the HIFI 1.2 THz wide spectral survey toward Orion KL. I. Methods
We present a comprehensive analysis of a broadband spectral line survey of the Orion
Kleinmann–Low nebula (Orion KL), one of the most chemically rich regions in the Galaxy …
Kleinmann–Low nebula (Orion KL), one of the most chemically rich regions in the Galaxy …
A line confusion limited millimeter survey of Orion KL I. Sulfur carbon chains-I. Sulfur carbon chains
B Tercero, J Cernicharo, JR Pardo… - Astronomy & …, 2010 - aanda.org
We perform a sensitive (line confusion limited), single-side band spectral survey towards
Orion KL with the IRAM 30 m telescope, covering the following frequency ranges: 80–115.5 …
Orion KL with the IRAM 30 m telescope, covering the following frequency ranges: 80–115.5 …
The ALMA view of the OMC1 explosion in orion
J Bally, A Ginsburg, H Arce, J Eisner… - The Astrophysical …, 2017 - iopscience.iop.org
Most massive stars form in dense clusters where gravitational interactions with other stars
may be common. The two nearest forming massive stars, the BN object and Source I …
may be common. The two nearest forming massive stars, the BN object and Source I …
Disk-driven rotating bipolar outflow in Orion Source I
T Hirota, MN Machida, Y Matsushita, K Motogi… - Nature …, 2017 - nature.com
One of the outstanding problems in star formation theory concerns the transfer of angular
momentum so that mass can accrete onto a newly born young stellar object (YSO). From a …
momentum so that mass can accrete onto a newly born young stellar object (YSO). From a …
Chasing discs around O-type (proto) stars-ALMA evidence for an SiO disc and disc wind from G17. 64+ 0.16
LT Maud, R Cesaroni, MSN Kumar… - Astronomy & …, 2018 - aanda.org
We present high angular resolution (~ 0.2 ″) continuum and molecular emission line
Atacama Large Millimeter/sub-millimeter Array (ALMA) observations of G17. 64+ 0.16 in …
Atacama Large Millimeter/sub-millimeter Array (ALMA) observations of G17. 64+ 0.16 in …
The Extraordinary Outburst in the Massive Protostellar System NGC 6334I-MM1: Flaring of the Water Masers in a North–South Bipolar Outflow Driven by MM1B
We compare multi-epoch sub-arcsecond Very Large Array imaging of the 22 GHz water
masers toward the massive protocluster NGC 6334I observed before and after the recent …
masers toward the massive protocluster NGC 6334I observed before and after the recent …
The mid-infrared molecular inventory toward Orion IRc2
S Nickerson, N Rangwala, SWJ Colgan… - The Astrophysical …, 2023 - iopscience.iop.org
We present the first high spectral resolution mid-infrared survey in the Orion BN/KL region,
covering 7.2–28.3 μm. With SOFIA/EXES, we target the enigmatic source Orion IRc2. While …
covering 7.2–28.3 μm. With SOFIA/EXES, we target the enigmatic source Orion IRc2. While …