O. S. Rojas-García
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View article: The LMT 2 millimeter receiver system (B4R). II. Science demonstration observations toward Orion-KL/OMC-1
The LMT 2 millimeter receiver system (B4R). II. Science demonstration observations toward Orion-KL/OMC-1 Open
We present the results of mapping and single-point spectral scans toward Orion-KL/OMC-1 performed as science demonstrations of a 2 mm superconductor–insulator–superconductor receiver, named the Band 4 Receiver (B4R), installed on the Large…
View article: Large-scale Mapping Observations of DCN and DCO<sup>+</sup> toward Orion KL
Large-scale Mapping Observations of DCN and DCO<sup>+</sup> toward Orion KL Open
We present emission maps ( scale, corresponding to 0.18 pc) of the DCN ( J = 2 − 1) and DCO + ( J = 2 − 1) lines in the 2 mm band toward the Orion KL region obtained with the 2 mm receiver system named B4R installed on the Large …
View article: Interstellar complex organic molecules towards outflows from the G351.16+0.70 (NGC 6334 V) massive protostellar system
Interstellar complex organic molecules towards outflows from the G351.16+0.70 (NGC 6334 V) massive protostellar system Open
G351.16+0.70 is a relatively well-studied high-mass star-forming region with at least two main bipolar outflow structures originating from an OB-embedded star and multiple IR sources. Using high-resolution and large-bandwidth SMA observati…
View article: Interstellar Complex Organic Molecules towards outflows from the G351.16+0.70 (NGC 6334 V) massive protostellar system
Interstellar Complex Organic Molecules towards outflows from the G351.16+0.70 (NGC 6334 V) massive protostellar system Open
G351.16+0.70 is a relatively well-studied High Mass Star Forming Region with at least two main bipolar outflow structures originating from an OB embedded star and multiple IR cores. Using high-resolution and large bandwidth SMA observation…
View article: Interstellar Complex Organic Molecules in SiO-traced Massive Outflows
Interstellar Complex Organic Molecules in SiO-traced Massive Outflows Open
The interstellar medium contains dust and gas, in which molecules can proliferate at high densities and in cold conditions. Interstellar complex organic molecules (iCOMs) are C-bearing species that contain at least six atoms. As they are d…
View article: Interstellar Complex Organic Molecules in SiO-traced massive outflows
Interstellar Complex Organic Molecules in SiO-traced massive outflows Open
The interstellar medium contains dust and gas, in which at high densities and cold conditions molecules can proliferate. Interstellar Complex Organic Molecules (iCOMs) are C-bearing species that contain at least six atoms. As they are dete…