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Table · dataset · 2000

Multiline CO observations of MBM 32

Listed in IVOA Registry (Virtual Observatory)

Using the KOSMA 3-m telescope we have made observations of the ^12^CO(J=1-0), (J=2-1) and (J=3-2), and the ^13^CO(J=1-0) and (J=2-1) transitions of the high latitude cloud MBM 32.

Description

The backend consisted of a Medium Resolution (channel width 167kHz; MRS), or a High Resolution (channel width 38.6kHz; HRS) acousto-optical Spectrometer. The following tables contain properties of clumps derived from the maps, assuming Gaussian clump parameters from the ^12^CO(J=1-0) MRS data (Table 3) ^12^CO(J=1-0) HRS data (Table 4) ^12^CO(J=2-1) MRS data (Table 5) ^13^CO(J=1-0) HRS data (Table 6).

We distinguish between different velocity components.

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Stated by source
Radio
Inferred from text
Tabular 65%
Provenance · 1 source records, 9 field assertions
SourceKeyLast seenRaw
IVOA Registry (Virtual Observatory)ivo://cds.vizier/j/a+as/144/12313 d agoJSON v1
FieldAssertionExtractorEvidence
access_levelsource · IVOA Registryconnector:ivoa_registry@1.0.0
concepts[field].local:field:astronomymapping · IVOA Registryconnector:ivoa_registry@1.0.0
concepts[modality].ivoa_waveband:radiosource · IVOA Registryconnector:ivoa_registry@1.0.0
concepts[modality].local:modality:tabularenrichment · IVOA Registrykeyword-concept-rules@1.0.0title+description (65%)
descriptionsource · IVOA Registryconnector:ivoa_registry@1.0.0rr.resource.res_description
license_textsource · IVOA Registryconnector:ivoa_registry@1.0.0
publication_datesource · IVOA Registryconnector:ivoa_registry@1.0.0
titlesource · IVOA Registryconnector:ivoa_registry@1.0.0rr.resource.res_title
updated_datesource · IVOA Registryconnector:ivoa_registry@1.0.0