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HD 142429


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The infrared void in the Lupus dark clouds revisited: a polarimetric approach
The results of B-band CCD imaging linear polarimetry obtained for starsfrom the Hipparcos catalogue are used to re-examine the distribution ofthe local interstellar medium towards the IRAS 100-μm emission voidin the Lupus dark clouds. The analysis of the obtainedparallax-polarization diagram assigns to the dark cloud Lupus1 adistance between 130 and 150pc and assures the existence of a low columndensity region coincident with the observed infrared void. Moreover,there are clear indications of the existence of absorbing material atdistances closer than 60-100pc, which may be associated with theinterface boundary between the Local Bubble and its neighbourhood LoopIsuperbubble.

Walraven photometry of nearby southern OB associations
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UBVRI photometry of FKSZ stars. II
The results of UBVRI photometry for 169 stars of the Faint FundamentalStars Catalog (Zverev, 1957) in the declination zone lambda of between-30 and -60 deg are presented. Observations were obtained between May1984 and February 1987 using the 50-cm ESO telescope at La Silla.Tabular data presented include the number of the star in the E-regions,the V magnitude, the (B-V), (U-B), (V-R), and (R-I) colors, and thespectral types.

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Observation and Astrometry data

Constellation:Lupus
Right ascension:15h55m50.57s
Declination:-35°40'33.6"
Apparent magnitude:7.796
Distance:166.113 parsecs
Proper motion RA:-22.8
Proper motion Dec:14.2
B-T magnitude:9.111
V-T magnitude:7.905

Catalogs and designations:
Proper Names
HD 1989HD 142429
TYCHO-2 2000TYC 7341-361-1
USNO-A2.0USNO-A2 0525-20786513
HIPHIP 78020

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