J/ApJ/899/55     Parameters of protoplanetary disks in 5 SFRs    (Aizawa+, 2020)

Search for Alignment of Disk Orientations in Nearby Star-forming Regions: Lupus, Taurus, Upper Scorpius, Aizawa M., Suto Y., Oya Y., Ikeda S., Nakazato T. <Astrophys. J., 899, 55 (2020)> =2020ApJ...899...55A 2020ApJ...899...55A
ADC_Keywords: Star Forming Region; Molecular clouds; YSOs; Interferometry; Optical; Radio sources Keywords: Protoplanetary disks ; Astrostatistics ; Interferometers ; Molecular clouds Abstract: Spatial correlations among protoplanetary disk orientations carry unique information on physics of multiple-star formation processes. We select five nearby star-forming regions that comprise a number of protoplanetary disks with spatially resolved images with ALMA and Hubble Space Telescope, and we search for the mutual alignment of the disk axes. Specifically, we apply the Kuiper test to examine the statistical uniformity of the position angle (PA: the angle of the major axis of the projected disk ellipse measured counterclockwise from the north) distribution. The disks located in the star-forming regions, except the Lupus clouds, do not show any signature of the alignment, supporting the random orientation. Rotational axes of 16 disks with spectroscopic measurement of PA in the LupusIII cloud, a subregion of the Lupus field, however, exhibit a weak and possible departure from the random distribution at a 2σ level, and the inclination angles of the 16 disks are not uniform as well. Furthermore, the mean direction of the disk PAs in the LupusIII cloud is parallel to the direction of its filament structure and approximately perpendicular to the magnetic field direction. We also confirm the robustness of the estimated PAs in the Lupus clouds by comparing the different observations and estimators based on three different methods, including sparse modeling. The absence of the significant alignment of the disk orientation is consistent with the turbulent origin of the disk angular momentum. Further observations are required to confirm/falsify the possible disk alignment in the Lupus III cloud. Description: In this paper, we focus on five nearby star-forming regions (Lupus, Taurus, Upper Scorpius, Ophiuchus and Orion) where many protoplanetary disks are spatially resolved with Atacama Large Millimeter/submillimeter Array (ALMA) and Hubble Space Telescope (HST), and search for the statistical signature of the alignment/nonuniformity of the PAs of the disks. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file tableb1.dat 82 37 *Parameters of disks in the Lupus region tableb2.dat 63 50 Parameters of disks in the Taurus region tableb3.dat 77 16 *Parameters of disks in the Upper Scorpius tableb4.dat 110 49 Parameters of disks in the Ophiuchus region tableb5.dat 43 31 *Parameters of disks or jets in ONC -------------------------------------------------------------------------------- Note on tableb1.dat : From Yen+, 2018A&A...616A.100Y 2018A&A...616A.100Y Note on tableb3.dat : From Barenfeld+, 2017ApJ...851...85B 2017ApJ...851...85B Note on tableb5.dat : From Bally+, 2000AJ....119.2919B 2000AJ....119.2919B -------------------------------------------------------------------------------- See also: II/332 : c2d Spitzer final data release (DR4) (Evans+, 2003) I/345 : Gaia DR2 (Gaia Collaboration, 2018) J/AJ/124/404 : Upper Scorpius OB association Li survey. II. (Preibisch, 2002) J/ApJ/651/L49 : Upper Sco OB association IRAC observations (Carpenter+, 2006) J/ApJS/177/551 : Spitzer c2d survey of Lupus dark clouds (Merin+, 2008) J/ApJS/181/321 : Properties of Spitzer c2d dark clouds (Evans+, 2009) J/MNRAS/402/1380 : Rotation velocities in Pleiades & αPer (Jackson+,2010) J/ApJ/743/54 : Polarization around star-forming regions (Targon+, 2011) J/ApJ/758/31 : IR photometry for members of Upper Sco (Luhman+, 2012) J/ApJ/746/154 : Improved kinematic plxes for Sco-Cen members (Pecaut+, 2012) J/ApJ/828/46 : ALMA survey of Lupus protoplanetary disks. I. (Ansdell+, 2016) J/ApJ/827/142 : ALMA observations of GKM stars in Upper Sco (Barenfeld+, 2016) J/ApJ/842/L9 : ALMA obs. polarized dust emission from Ser-emb 8 (Hull+, 2017) J/ApJ/859/21 : ALMA survey of Lupus protoplanetary disks. II. (Ansdell+,2018) J/A+A/612/L2 : Compilation of stellar rotation data (Kovacs, 2018) J/A+A/618/A109 : Seismic global parameters of 372 KIC (Mosser+, 2018) J/MNRAS/482/698 : Ophiuchus DIsc Survey Employing ALMA. I. (Cieza+,2019) Byte-by-byte Description of file: tableb1.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 17 A17 --- Source Source name 19- 27 F9.5 deg RAdeg [234.8/242.8] Right Ascension (J2000) 29- 37 F9.5 deg DEdeg [-42.4/-34.2] Declination (J2000) 39- 41 I3 deg PA [25/355] Position Angle 43- 44 I2 deg E_PA [5/40] Upper error on PA 46- 47 I2 deg e_PA [5/40] Lower error on PA 49- 49 A1 --- l_i [<]? limit flag on i 51- 52 I2 deg i [15/75] inclination angle 54- 55 I2 deg E_i [5/10]? Upper error on i 57- 58 I2 deg e_i [5/20]? Lower error on i 60- 64 F5.1 pc X [-73.4/-48.3] Projected location, in X direction 66- 71 F6.1 pc Y [-133/-91.6] Projected location, in Y direction 73- 78 F6.1 pc Z [-122/-84.6] Projected location, in Z direction 80- 82 A3 --- Lupus In Lupus III? -------------------------------------------------------------------------------- Byte-by-byte Description of file: tableb2.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 11 A11 --- Source Source name 13- 20 F8.5 deg RAdeg [64.3/84] Right Ascension (J2000) 22- 29 F8.5 deg DEdeg [16.9/30.8] Declination (J2000) 31- 35 F5.1 deg PA [4.0/179.1] Position Angle 37- 40 F4.1 deg e_PA [0.0/28.0] Symmetric error on PA 42- 45 F4.2 --- cosi [0.15/0.98] cosine, inclination angle 47- 50 F4.2 --- e_cosi [0.0/0.3] Symmetric error on cosi 52- 55 F4.2 arcsec rdisk [0.03/6.2] Disk Radius, arcseconds 57- 60 F4.2 arcsec e_rdisk [0.0/0.7]? Symmetric error on rdisk 62- 63 I2 --- Ref [1/5] References (1) -------------------------------------------------------------------------------- Note (1): References as follows: 1 = Kitamura+, 2002ApJ...581..357K 2002ApJ...581..357K 2 = Andrews & Williams, 2007ApJ...659..705A 2007ApJ...659..705A 3 = Guilloteau+, 2011A&A...529A.105G 2011A&A...529A.105G 4 = Long+, 2018ApJ...869...17L 2018ApJ...869...17L 5 = Long+, 2019ApJ...882...49L 2019ApJ...882...49L -------------------------------------------------------------------------------- Byte-by-byte Description of file: tableb3.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 23 A23 --- Source Source name 25- 33 F9.5 deg RAdeg [238.4/246.8] Right Ascension (J2000) 35- 43 F9.5 deg DEdeg [-25.4/-18.9] Declination (J2000) 45- 47 I3 deg PA [0/176] Position Angle 49- 50 I2 deg E_PA [3/36] Upper error on PA 52- 53 I2 deg e_PA [2/31] Lower error on PA 55- 56 I2 deg i [27/89] inclination angle 58- 59 I2 deg E_i [1/21] Upper error on i 61- 62 I2 deg e_i [2/36] Lower error on i 64- 67 F4.2 arcsec rdisk [0.08/0.82] Disk Radius, arcseconds 69- 72 F4.2 arcsec E_rdisk [0.01/0.63] Upper error on rdisk 74- 77 F4.2 arcsec e_rdisk [0.01/0.33] Lower error on rdisk -------------------------------------------------------------------------------- Byte-by-byte Description of file: tableb4.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 25 A25 --- Source Source name 27- 40 A14 --- OName Other name 42- 50 F9.5 deg RAdeg [245.3/250] Right Ascension (J2000) 52- 60 F9.5 deg DEdeg [-25/-23] Declination (J2000) 62- 66 F5.1 deg PA1 [0.1/177]? Position Angle, Cox+, 2017ApJ...851...83C 2017ApJ...851...83C 68- 71 F4.1 deg e_PA1 [0.2/28.0]? Symmetric error on PA1 73- 77 F5.1 deg PA2 [14.2/174.2]? Position Angle, Cieza+, 2019, J/MNRAS/482/698 79- 82 F4.1 deg e_PA2 [0.0/18.0]? Symmetric error on PA2 84- 88 F5.3 --- cosi [0.1/0.924] cosine, inclination angle (1) 90- 94 F5.3 --- e_cosi [0.002/0.355] Symmetric error on cosi (1) 96-100 F5.3 arcsec rdisk [0.035/0.65] Disk Radius, arcseconds (1) 102-106 F5.3 arcsec e_rdisk [0.001/0.059] Symmetric error on rdisk (1) 108-110 A3 --- L1688 In L1688? -------------------------------------------------------------------------------- Note (1): We list values in Cox+, 2017ApJ...851...83C 2017ApJ...851...83C. If the values in Cox+ are not available, we use values in Cieza+, 2019, J/MNRAS/482/698. -------------------------------------------------------------------------------- Byte-by-byte Description of file: tableb5.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 7 A7 --- Source Source name 9- 9 A1 --- f_PA Flag on PA (1) 11- 18 F8.5 deg RAdeg [83.7/83.9] Right Ascension (J2000) 20- 27 F8.5 deg DEdeg [-5.44/-5.3] Declination (J2000) 29- 33 F5.1 deg PA [0.0/176.0] Position Angle 35- 38 F4.2 --- cosi [0.2/0.71]? cosine, inclination angle 40- 43 F4.2 arcsec rdisk [0.15/1.35]? Disk Radius -------------------------------------------------------------------------------- Note (1): Flag as follows: a = PA is estimated from orientations of jets (19 occurrences) -------------------------------------------------------------------------------- History: From electronic version of the journal
(End) Prepared by [AAS], Coralie Fix [CDS], 14-Oct-2021
The document above follows the rules of the Standard Description for Astronomical Catalogues; from this documentation it is possible to generate f77 program to load files into arrays or line by line