J/MNRAS/476/4442    Polarization of seven MBM clouds stars         (Neha+, 2018)

Polarization of seven MBM clouds at high Galactic latitude. Neha S., Maheswar G., Soam A., Lee C.W. <Mon. Not. R. Astron. Soc., 476, 4442-4458 (2018)> =2018MNRAS.476.4442N 2018MNRAS.476.4442N (SIMBAD/NED BibCode)
ADC_Keywords: Molecular clouds ; Magnetic fields ; Polarization Keywords: polarization - ISM: clouds - ISM: individual objects: MBM 33-39 - ISM: magnetic fields Abstract: We made R-band polarization measurements of 234 stars towards the direction of the MBM 33-39 cloud complex. The distance of the MBM 33-39 complex was determined as 120±10pc using polarization results and near-infrared photometry from the 2MASS survey. The magnetic field geometry of the individual clouds inferred from our polarimetric results reveals that the field lines are in general consistent with the global magnetic field geometry of the region obtained from previous studies. This implies that the clouds in the complex are permeated by the interstellar magnetic field. Multi-wavelength polarization measurements of a few stars projected on to the complex suggest that the size of the dust grains in these clouds is similar to those found in the normal interstellar medium of the Milky Way. We studied a possible formation scenario of the MBM 33-39 complex by combining the polarization results from our study with those from the literature and by identifying the distribution of ionized, atomic and molecular (dust) components of material in the region. Description: Polarimetric observations were made using the Aries Imaging Polarimeter (AIMPOL). This polarimeter is used as a back-end instrument at the Cassegrain focus of the 104-cm Sampurnanand Telescope, which is at the Aryabhatta Research Institute of Observational Sciences (ARIES), Nainital, India. We also observed a few bright stars towards MBM 33, MBM 34 and MBM 35 in multi-wavelengths (V, R and I). File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table6.dat 100 30 Polarization of observed Tycho stars in the VRI filters table7.dat 59 234 Polarization results of 234 stars observed in the direction of the MBM 33-39 cloud complex with P/σP≥2 -------------------------------------------------------------------------------- Byte-by-byte Description of file: table6.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 6 A6 --- Cluster Cluster name, MBM 33, MBM 34 and MBM 35 8- 9 I2 --- Star [1/30] Star ID 11- 20 F10.6 deg RAdeg Right ascension (J2000) 22- 30 F9.6 deg DEdeg Declination (J2000) 32- 34 F3.1 % PV Polarisation degree in V band 36- 38 F3.1 % e_PV rms uncertainty on PV 40- 41 I2 deg thetaV Polarisation angle in V band 43 I1 deg e_thetaV rms uncertainty on thetaV 45- 47 F3.1 % PR Polarisation degree in R band 49- 51 F3.1 % e_PR rms uncertainty on PR 53- 54 I2 deg thetaR Polarisation angle in R band 56 I1 deg e_thetaR rms uncertainty on thetaR 58- 60 F3.1 % PI Polarisation degree in I band 62- 64 F3.1 % e_PI rms uncertainty on PI 66- 68 I3 % thetaI Polarisation angle in I band 70 I1 % e_thetaI rms uncertainty on thetaI 72- 75 F4.2 % lambdamax Wavelenght of maximum degree of polarization 77- 80 F4.2 % e_lambdamax rms uncertainty on lambdamax 82- 85 F4.2 um Pmax Maximum degree of polarization as a percentage at wavelength lambdamax 87- 90 F4.2 um e_Pmax rms uncertainty on Pmax 92- 95 F4.2 -- RV Total-to-selective extinction 97-100 F4.2 --- e_RV rms uncertainty on RV -------------------------------------------------------------------------------- Byte-by-byte Description of file: table7.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 3 I3 --- Star [1/234] Star ID 5- 14 F10.6 deg RAdeg Right ascension (J2000) 16- 24 F9.6 deg DEdeg Declination (J2000) 26- 32 F7.3 deg GLON Galactic longitude 34- 39 F6.3 deg GLAT Galactic latitude 41- 43 F3.1 % P Degree of polarization 45- 48 F4.2 % e_P rms uncertainty on P 50- 52 I3 deg theta Polarization position angle 54- 55 I2 deg e_theta rms uncertainty on theta 57- 59 I3 deg thetaGal Galactic polarization position angle measured from Galactic North -------------------------------------------------------------------------------- History: From electronic version of the journal
(End) Patricia Vannier [CDS] 27-Apr-2021
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