The large globule LYNDS 810 as a possible member of the Vulpecula OB1 complex

Details The large globule LYNDS 810 as a possible member of the Vulpecula OB1 complex The large globule LYNDS 810 as a possible member of the Vulpecula OB1 complex

Oct 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986a%26a...167..157t&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 167, no. 1, Oct. 1986, p. 157-160.

Astronomy and Astrophysics

Astrophysics

20

Cometary Atmospheres, Globular Clusters, Interstellar Gas, Molecular Clouds, Stellar Spectrophotometry, Ubv Spectra, Dwarf Stars, H Ii Regions, Radial Velocity, Stellar Winds

Scientific paper

A distance of 2.5±0.2 kpc is derived for the dark globule Lynds 810 using photometric data for foreground stars and star counts. It is argued that this globule is likely to belong to the Vul OB1 complex. Its cometary structure, like certain other features of dust-related objects in Vulpecula, appears to be the shock signature of a past disturbance originating from a region near l = 60°, b = +2°, which lies within the fossil H II region Lynds 792.

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