Add to ORKGThe detection of a predicted transition, the fine structure line of O3 at 88.16 microns in the H 2 region M17, was reported. Line intensity was measured at 2.2 sub + 7 sub -0.7 times 10 to the 15th power
We report the first measurements of the interstellar J = 3 to J = 2 carbon monoxide line at a wavele...
Far infrared fine structure line data from the ISO archive have been extracted for several hundred Y...
We have made the first detections of the 88 micrometers [O(sub III)] line from galaxies in the early...
The (0 III) 51.8 microns line from four H II regions, M42, M17, W51 and NGC 6375A was detected. Resp...
Observations of the O III 88.35 micrometer line and the O I63.2 micrometer were made with a far infr...
The 51.8 micron fine structure transition P2:3P2 3P1 for doubly ionized oxygen was observed in the O...
We investigate the origin of self-absorption in [O I] 63 mu m line emission, which is very clearly s...
Galactic (C II) 157 micron, fine-structure emission was estimated. At a Galactic longitude of 8 deg,...
The first astronomical detection of the metastable ($J,K$) = (18,18) line of NH3 is reported. With 3...
The pure rotational S(2) line of molecular hydrogen at 12.28 microns was looked for in 44 positions ...
The O i 135.56 nm line is covered by NASA's Interface Region Imaging Spectrograph (IRIS) small explo...
The 63 micrometer (3)p(1)-(3)P(2) fine structure line emission of neutral atomic oxygen at the cente...
Context. The discovery of a broad, ∼1.5° long filamentary [OIII] 5007 emission ∼1.2° south-east of t...
Far infrared fine structure line data from the ISO archive have been extracted for several hundred Y...
International audienceWe report the first detections of the [N II] 122 mum line from a high-redshift...
We report the first measurements of the interstellar J = 3 to J = 2 carbon monoxide line at a wavele...
Far infrared fine structure line data from the ISO archive have been extracted for several hundred Y...
We have made the first detections of the 88 micrometers [O(sub III)] line from galaxies in the early...
The (0 III) 51.8 microns line from four H II regions, M42, M17, W51 and NGC 6375A was detected. Resp...
Observations of the O III 88.35 micrometer line and the O I63.2 micrometer were made with a far infr...
The 51.8 micron fine structure transition P2:3P2 3P1 for doubly ionized oxygen was observed in the O...
We investigate the origin of self-absorption in [O I] 63 mu m line emission, which is very clearly s...
Galactic (C II) 157 micron, fine-structure emission was estimated. At a Galactic longitude of 8 deg,...
The first astronomical detection of the metastable ($J,K$) = (18,18) line of NH3 is reported. With 3...
The pure rotational S(2) line of molecular hydrogen at 12.28 microns was looked for in 44 positions ...
The O i 135.56 nm line is covered by NASA's Interface Region Imaging Spectrograph (IRIS) small explo...
The 63 micrometer (3)p(1)-(3)P(2) fine structure line emission of neutral atomic oxygen at the cente...
Context. The discovery of a broad, ∼1.5° long filamentary [OIII] 5007 emission ∼1.2° south-east of t...
Far infrared fine structure line data from the ISO archive have been extracted for several hundred Y...
International audienceWe report the first detections of the [N II] 122 mum line from a high-redshift...
We report the first measurements of the interstellar J = 3 to J = 2 carbon monoxide line at a wavele...
Far infrared fine structure line data from the ISO archive have been extracted for several hundred Y...
We have made the first detections of the 88 micrometers [O(sub III)] line from galaxies in the early...