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J/A+A/384/1050 Interstellar polarization. VI. (Berdyugin+, 2002)
Interstellar polarization at high galactic latitudes from distant stars. VI. Extended polarization map and connection with the local spiral structure. Berdyugin A., Teerikorpi P. <Astron. Astrophys. 384, 1050 (2002)> =2002A&A...384.1050B
ADC_Keywords: Polarization ; Galactic pole, north Keywords: polarization - ISM: dust, extinction - Galaxy: structure - Galaxy: general Abstract: We present new interstellar polarization measurements for 116 stars at high galactic latitudes. Our data show that Markkanen's cloud - the main polarization structure seen in the North Galactic Pole area (b>75°) extends further towards lower latitudes. Especially, we have found a new dust formation in the area 35°<l<45°, 57°<b<63°. Interstellar polarization in this part of the sky peaks at 0.7%, which gives a lower limit to the extinction AV>0.23mag. Polarization vectors in this cloud are very well aligned along the direction of l=50°. On the IRAS 100 micron map this dust structure shows up as a bright emission area. We discuss the new polarization map extending from circumpolar to lower latitudes and point out features which suggest that Markkanen's cloud may be a part of the dust lane in the inner edge of the local spiral or spur. File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file table1.dat 52 102 New polarization measurements
See also: J/A+A/372/276 : Polarization catalogue for NGP area (Berdyugin+, 2001) Byte-by-byte Description of file: table1.dat
Bytes Format Units Label Explanations
1- 9 A9 --- BD BD number of the star 11- 14 F4.2 % Pol Polarization percentage. 16 I1 --- r_Pol [1-2] Source of data (1) 18- 21 F4.2 % e_Pol Error of polarization measurement 23- 25 I3 deg theta ? Position angle of polarization vector measured in the equatorial coordinate frame 27- 28 I2 deg e_theta ? Error of position angle measurement 30- 32 I3 pc Dist Distance to the star 34- 39 F6.2 deg GLON Galactic longitude 41- 45 F5.2 deg GLAT Galactic latitude 47- 51 A5 --- SpType Spectral type, when available
Note (1): Source of polarisation data: 1: from the KVA 60 cm telescope 2: from the NOT 2.56 m telescope
History: * 08-Jun-2002: the BD number originally written "+91 2793" was corrected to "+19 2793" Acknowledgements: Andrei Berdyugin Acknowledgements: Andrei Berdyugin References: Berdyugin et al., Paper I 1995A&A...294..568B Berdyugin & Teerikorpi, Paper II 1997A&A...318...37B Berdyugin et al., Paper III 2000A&A...358..717B Berdyugin et al., Paper IV 2001A&A...372..276B, Cat. J/A+A/372/276 Berdyugin & Teerikorpi, Paper V 2001A&A...368..635B
(End) Patricia Bauer [CDS] 15-Mar-2002
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