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HD 103216 (Kazantseva Anastasia)


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FAUST observations near the North Galactic Pole
We analyse a UV observation with FAUST in the direction of the NorthGalactic Pole. The region includes a cirrus cloud (G251.2+73.3) and adark globule, and the FAUST image contains 75 UV sources. We discuss theUV source detection and their identification with optical counterparts.We use, for the first time, low-resolution spectral information as theprimary means of identifying possible optical counterparts. This iscomplemented, and sometimes modified, by optical information availablefrom existing data bases. The results are interpreted with the help ofmaps of the distribution of far-infrared emission and of the neutralhydrogen gas. We discuss the types of objects found, the degree ofmatching with the predictions of our UV Galaxy model, and the generalbehaviour of the Galactic UV extinction in this Milky Way part. Wecompare the UV results for this region with similar observations in thesame neighbourhood, which are less affected by dust, and attempt toexplain the peculiar distribution of UV magnitudes as a result of apeculiar distribution of foreground dust, which does not follow theaccepted dust-to-gas relation.

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Observation and Astrometry data

Constellation:Leo
Right ascension:11h53m10.88s
Declination:+16°50'56.4"
Apparent magnitude:8.613
Distance:152.672 parsecs
Proper motion RA:-49.2
Proper motion Dec:-17.9
B-T magnitude:9.061
V-T magnitude:8.65

Catalogs and designations:
Proper NamesKazantseva Anastasia
  (Edit)
HD 1989HD 103216
TYCHO-2 2000TYC 1441-1506-1
USNO-A2.0USNO-A2 1050-06602423
HIPHIP 57952

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