Add to ORKGA new complex of infrared sources ~1' across has been discovered in Orion. Associated with this cluster is an extended ~6' molecular cloud producing intense CO emission. Its measured infrared luminosity is less than ~500 L_☉. The complex is hypothesized to be composed of pre-main-sequence sources. Several arguments suggest that these stars heat dust in the larger molecular cloud and thus cause the strong CO emission. The complex is not associated with a known visible or radio continuum feature, and searches over a 0.º7 X 0.º7 field show no other comparable unknown 2.2-μ sources
We present ALMA observations of the largest protoplanetary disk in the Orion Nebula, 114–426. Detect...
The J = 1 → 0 emission of CO has been surveyed in the galactic plane between ℓ = -10° and +90° with ...
Regions of massive star formation have long been believed to have a profound influence on the struct...
A new complex of infrared sources ~1' across has been discovered in Orion. Associated with this clus...
Recent infrared and radio spectroscopic data pertaining to the Orion BN-KL infrared cluster are revi...
We present a 1".3 spatial resolution interferometric spectral line survey of the core of the Orion m...
A preliminary CO emission line survey covering a strip at b = -2' from ℓ = 359°.7 to ℓ = 2°.8 is pre...
We report the first measurements of the interstellar J = 3 to J = 2 carbon monoxide line at a wavele...
We have observed the central region of the infrared-dark cloud filament associated with IRAS 18507+0...
The Orion Nebula was the subject of intensive study for over one hundred years. Recently, several fa...
The far-infrared IRAS 15507-5359 source is known to be a medium-mass star-forming region associated ...
Context. The Orion-KL region contains the closest examples of high-mass accretion disk candidates. ...
The results of a submillimetre wavelength spectral line survey between 455.1-507.4 GHz of the Orion-...
We detail tentative detections of low-frequency carbon radio recombination lines from within the Ori...
JOURThis is the final version of the article. It was first published by Oxford Journals for the Roya...
We present ALMA observations of the largest protoplanetary disk in the Orion Nebula, 114–426. Detect...
The J = 1 → 0 emission of CO has been surveyed in the galactic plane between ℓ = -10° and +90° with ...
Regions of massive star formation have long been believed to have a profound influence on the struct...
A new complex of infrared sources ~1' across has been discovered in Orion. Associated with this clus...
Recent infrared and radio spectroscopic data pertaining to the Orion BN-KL infrared cluster are revi...
We present a 1".3 spatial resolution interferometric spectral line survey of the core of the Orion m...
A preliminary CO emission line survey covering a strip at b = -2' from ℓ = 359°.7 to ℓ = 2°.8 is pre...
We report the first measurements of the interstellar J = 3 to J = 2 carbon monoxide line at a wavele...
We have observed the central region of the infrared-dark cloud filament associated with IRAS 18507+0...
The Orion Nebula was the subject of intensive study for over one hundred years. Recently, several fa...
The far-infrared IRAS 15507-5359 source is known to be a medium-mass star-forming region associated ...
Context. The Orion-KL region contains the closest examples of high-mass accretion disk candidates. ...
The results of a submillimetre wavelength spectral line survey between 455.1-507.4 GHz of the Orion-...
We detail tentative detections of low-frequency carbon radio recombination lines from within the Ori...
JOURThis is the final version of the article. It was first published by Oxford Journals for the Roya...
We present ALMA observations of the largest protoplanetary disk in the Orion Nebula, 114–426. Detect...
The J = 1 → 0 emission of CO has been surveyed in the galactic plane between ℓ = -10° and +90° with ...
Regions of massive star formation have long been believed to have a profound influence on the struct...