J/A+AS/144/195      UBVRI polarimetric observations in NGC 6611 (Orsatti+, 2000)

Dust properties in NGC 6611 Orsatti A.M., Vega E.I., Marraco H.G. <Astron. Astrophys. Suppl. Ser. 144, 195 (2000)> =2000A&AS..144..195O 2000A&AS..144..195O
ADC_Keywords: Clusters, open ; Polarization ; Photometry, UBVRI Keywords: dust - extinction - ISM: HII regions - ISM: magnetic fields - Galaxy: open clusters and associations: individual: NGC 6611 Abstract: An investigation on dust properties in the NW portion of NGC 6611 has been conducted polarimetrically to test the existence of abnormal extinction in that section of the open cluster in an independent way. As previously suggested for the η Carinae nebula by Tapia et al. (1988, in Conference on Dust in the Universe, Bailey M.E. and Williams D.A. (eds.) Cambridge University Press, Cambridge, p.19) and subsequently confirmed by Marraco et al. (1993), the canonical relation between EV-K/EB-V and λmax (the wavelength of maximum interstellar polarization) is not valid for stars belonging to dusty HII regions, as is the case for the observed portion of M 16. This may arise mainly from the presence of silicate grains of a slightly larger size than the standard ISM and also from a considerable increase in mean graphite grain size, according to previous results from Chini & Wargau (1990A&A...227..213C 1990A&A...227..213C). About 50% of the observed stars in NGC 6611 present indications of intrinsic polarization in their measurements; a similar percentage was found in IC 2944 (Vega et al., 1994AJ....108.1834V 1994AJ....108.1834V), another young open cluster in close relation with an HII region. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file object.dat 26 39 Object positions from Simbad table1.dat 81 195 UBVRI polarimetric observations table1.tex 103 397 LaTeX version of table1 -------------------------------------------------------------------------------- See also: J/A+AS/134/525 : NGC 6611 compiled catalog (Belikov+ 1999) J/A+AS/121/223 : Multiphotometry of NGC 6611 (de Winter+ 1997) Byte-by-byte Description of file: object.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 3 I3 --- NGC6611 Star number (Walker, 1961ApJ...133..438W 1961ApJ...133..438W) 6- 7 I2 h RAh Right ascension (J2000.0) 9- 10 I2 min RAm Right ascension (J2000.0) 12- 15 F4.1 s RAs Right ascension (J2000.0) 17 A1 --- DE- Declination sign (J2000.0) 18- 19 I2 deg DEd Declination (J2000.0) 21- 22 I2 arcmin DEm Declination (J2000.0) 24- 25 I2 arcsec DEs Declination (J2000.0) -------------------------------------------------------------------------------- Byte-by-byte Description of file: table1.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 3 I3 --- NGC6611 Star number (Walker, 1961ApJ...133..438W 1961ApJ...133..438W) NGC 6611 NNN in Simbad 4 A1 --- f_NGC6611 [*] *: star considered as being "frontside" 6- 32 A27 --- Name HD, BD or H designation (1) 34 A1 --- Band [UBVRI] Band (2) 36- 40 F5.2 % Pol Observed percentage polarisation 42- 45 F4.2 % e_Pol rms uncertainty on Pol 47- 51 F5.1 deg PA Observed position angle of the electric vector 53- 56 F4.1 deg e_PA rms uncertainty on PA 58- 59 I2 --- n ? Number of integrations 61- 64 F4.2 % PolI ? Intracluster percentage polarisation 66- 69 F4.2 % e_PolI ? rms uncertainty on PolI 71- 75 F5.1 deg PAI ? Intracluster position angle of the electric vector 77- 81 F5.2 deg e_PAI ? rms uncertainty on PAI -------------------------------------------------------------------------------- Note (1): Identifications from Henry Draper, Cat. III/135, Bonner Durchmusterung, Cat. I/122 or Hoag et al., 1961PUSNO..17..343H 1961PUSNO..17..343H. Note (2): Wavelengths of the bands for which Pol and PA are measured: U: 0.360µm B: 0.440µm V: 0.53µm R: 0.690µm I: 0.830µm -------------------------------------------------------------------------------- Acknowledgements: Hugo Marraco
(End) Patricia Bauer [CDS] 04-May-2000
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