J/ApJ/833/18     Ultra-compact HII regions & methanol masers. I.     (Hu+, 2016)

On the relationship of UC HII regions and class II methanol masers. I. Source catalogs. Hu B., Menten K.M., Wu Y., Bartkiewicz A., Rygl K., Reid M.J., Urquhart J.S., Zheng X. <Astrophys. J., 833, 18-18 (2016)> =2016ApJ...833...18H 2016ApJ...833...18H (SIMBAD/NED BibCode)
ADC_Keywords: Masers ; H II regions ; Radio continuum ; Radial velocities Keywords: catalogs; ISM: molecules; masers; stars: formation Abstract: We conducted Very Large Array C-configuration observations to measure positions and luminosities of Galactic Class II 6.7GHz methanol masers and their associated ultra-compact HII regions. The spectral resolution was 3.90625kHz and the continuum sensitivity reached 45µJy/beam. We mapped 372 methanol masers with peak flux densities of more than 2Jy selected from the literature. Absolute positions have nominal uncertainties of 0.3". In this first paper on the data analysis, we present three catalogs; the first gives information on the strongest feature of 367 methanol maser sources, and the second provides information on all detected maser spots. The third catalog presents derived data of the 127 radio continuum counterparts associated with maser sources. Our detection rate of radio continuum counterparts toward methanol masers is approximately one-third. Our catalogs list properties including distance, flux density, luminosity, and the distribution in the Galactic plane. We found no significant relationship between luminosities of masers and their associated radio continuum counterparts, however, the detection rate of radio continuum emission toward maser sources increases statistically with the maser luminosities. Description: 372 unique targets were selected from the following methanol maser surveys: the Methanol Multi-Beam catalog (MMB; Caswell & Breen 2010MNRAS.407.2599C 2010MNRAS.407.2599C; Green+ 2010-2012, VIII/96), the Arecibo Methanol Maser Galactic Plane Survey (AMGPS; Pandian+ 2011ApJ...730...55P 2011ApJ...730...55P), the Torun catalog of 6.7GHz methanol masers (Szymczak+ 2012, J/AN/333/634), and other individual observations of known 6.7GHz methanol masers or MSFRs (Caswell+ 1995MNRAS.272...96C 1995MNRAS.272...96C; Walsh+ 1997, J/MNRAS/291/261; 1998, J/MNRAS/301/640; Xu+ 2008A&A...485..729X 2008A&A...485..729X; Caswell 2009, J/other/PASA/26.454). The observations were conducted with the VLA in C-configuration using five sessions from 2012 February 28 to April 16. Spectral line data used 2048 channels across 8MHz, yielding a channel spacing of 3.90625kHz at the central frequency of 6.6685192GHz and a velocity resolution of 0.176km/s. The continuum observations employed two 1GHz sub-bands from 4.9840 to 6.0080GHz (the low band) and from 6.6245 to 7.6485GHz (the high band) and each sub-band was divided into 16 channels. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table2.dat 43 33 Non-detection sources table3.dat 86 367 6.7GHz methanol maser catalog (corrected version from the author) table4.dat 86 8971 The maser spots catalog (corrected version from the author) table5.dat 85 279 Catalog of radio continuum counterpart of maser sources -------------------------------------------------------------------------------- See also: VIII/96 : 6-GHz methanol multibeam maser catalogue (Caswell+, 2010-12) J/MNRAS/446/3461 : 6.7-GHz methanol masers-dust associations (Urquhart+, 2015) J/ApJ/783/130 : Parallaxes of high mass star forming regions (Reid+, 2014) J/A+A/563/A130 : GLIMPSE/BGPS 6.7GHz methanol maser survey (Sun+, 2014) J/other/IJAA/4.571 : Methanol masers in HII regions (Farmer, 2014) J/MNRAS/435/400 : ATLASGAL. Compact HII regions properties (Urquhart+, 2013) J/ApJS/205/1 : CORNISH project. II. Source catalog (Purcell+, 2013) J/A+A/549/A45 : ATLASGAL Compact Source Catalog: 330<l<21 (Contreras+, 2013) J/AN/333/634 : Torun methanol source catalogue (Szymczak+, 2012) J/ApJS/194/25 : VLBA calibrator search for the BeSSeL survey (Immer+, 2011) J/other/PASA/26.454 : Precise positions of methanol masers (Caswell, 2009) J/A+A/501/539 : RMS survey. 6cm observations of YSOs (Urquhart+, 2009) J/AJ/136/2391 : GLIMPSE Extended Green Objects catalog (Cyganowski+, 2008) J/ApJ/656/255 : Arecibo methanol maser Gal. Plane Survey (Pandian+, 2007) J/A+A/453/1003 : SCUBA ultracompact HII regions (Thompson+, 2006) J/A+A/403/1095 : 6.7GHz methanol masers survey of YSOs (Minier+, 2003) J/MNRAS/301/640 : Ultracompact H II regions studies. II. (Walsh+, 1998) J/MNRAS/291/261 : Methanol maser of IRAS-selected sources (Walsh+ 1997) Byte-by-byte Description of file: table2.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 12 A12 --- Name Source name (GLLL.ll+B.bb) 15- 16 I2 h RAh Hour of Right Ascension (J2000) 18- 19 I2 min RAm Minute of Right Ascension (J2000) 21- 26 F6.3 s RAs Second of Right Ascension (J2000) 27 A1 --- DE- Sign of the Declination (J2000) 28- 29 I2 deg DEd Degree of Declination (J2000) 31- 32 I2 arcmin DEm Arcminute of Declination (J2000) 34- 38 F5.2 arcsec DEs Arcsecond of Declination (J2000) 40- 43 A4 --- Ref Reference (1) -------------------------------------------------------------------------------- Note (1): References as follows: C10 = Caswell & Breen (2010MNRAS.407.2599C 2010MNRAS.407.2599C); G10 = Green et al. (2010MNRAS.409..913G 2010MNRAS.409..913G; see VIII/96); S14 = Sun et al. (2014, J/A+A/563/A130); SZ12 = Szymczak et al.(2012, J/AN/333/634); W97 = Walsh et al. (1997, J/MNRAS/291/261); X09 = Xu et al. (2009A&A...507.1117X 2009A&A...507.1117X). -------------------------------------------------------------------------------- Byte-by-byte Description of file: table3.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 14 A14 --- Name Source name (GLLL.lll+B.bbb) 16- 17 I2 h RAh Hour of Right Ascension (J2000) 19- 20 I2 min RAm Minute of Right Ascension (J2000) 22- 27 F6.3 s RAs Second of Right Ascension (J2000) 29- 29 A1 --- DE- Sign of the Declination (J2000) 30- 31 I2 deg DEd Degree of Declination (J2000) 33- 34 I2 arcmin DEm Arcminute of Declination (J2000) 36- 40 F5.2 arcsec DEs Arcsecond of Declination (J2000) 42- 47 F6.2 km/s Vlsr [-70/153] Local Standard of Rest (LSR) velocity of strongest maser spot 49- 53 F5.2 km/s DelV [0.1/21] Velocity range of maser ΔV 55- 61 F7.2 Jy/beam Spk [0.2/3629] Peak flux density 63- 70 F8.2 Jy Sint [0.4/37475] Integrated flux density 72- 75 F4.1 kpc Dist [0.6/17] Heliocentric distance 77- 79 F3.1 kpc e_Dist [0/3] Uncertainty in Dist 81- 84 F4.2 --- Prob Probability source is at Distance, Dist (see section 5.2 for details) 86- 86 A1 --- Code Association code between maser source and the continuum emission (G1) -------------------------------------------------------------------------------- Byte-by-byte Description of file: table4.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 14 A14 --- Name Source name (GLLL.lll+B.bbb) 16- 17 I2 h RAh Hour of Right Ascension (J2000) of reference position 19- 20 I2 min RAm Minute of Right Ascension (J2000) 22- 27 F6.3 s RAs Second of Right Ascension (J2000) 29- 29 A1 --- DE- Sign of the Declination (J2000) of reference position 30- 31 I2 deg DEd Degree of Declination (J2000) of reference position 33- 34 I2 arcmin DEm Arcminute of Declination (J2000) 36- 40 F5.2 arcsec DEs [0/60] Arcsecond of Declination (J2000) 42- 48 F7.2 km/s Vlsr [-72/159] Radial Velocity of maser spot 50- 56 F7.2 Jy/beam Spk [0.08/3629] Peak Flux of maser spot, Jansky 58- 65 F8.3 arcsec dX X offset to maser spot from reference position 67- 71 F5.3 arcsec e_dX Uncertainty in X offset 73- 80 F8.3 arcsec dY Y offset to maser spot from reference position 82- 86 F5.3 arcsec e_dY Uncertainty in Y offset -------------------------------------------------------------------------------- Byte-by-byte Description of file: table5.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 14 A14 --- Name Source name (GLLL.lll+B.bbb) 16- 17 I2 h RAh Hour of Right Ascension (J2000) 19- 20 I2 min RAm Minute of Right Ascension (J2000) 22- 26 F5.2 s RAs Second of Right Ascension (J2000) 28- 28 A1 --- DE- Sign of the Declination (J2000) 29- 30 I2 deg DEd Degree of Declination (J2000) 32- 33 I2 arcmin DEm Arcminute of Declination (J2000) 35- 38 F4.1 arcsec DEs Arcsecond of Declination (J2000) 40- 46 F7.2 mJy Fint [0.1/9300] Integrated flux of the entire continuum source 48- 53 F6.2 --- I/P [0.1/562] Ratio of integrated flux to peak pixel value 55- 59 F5.1 arcsec a Source elliptical shape parameter, a 61- 65 F5.1 arcsec b Source elliptical shape parameter, b 67- 71 F5.1 deg PA Source elliptical shape parameter, position angle 73- 76 F4.2 pc Offset [0/7] Displacement between peaks of maser and continuum sources 78- 78 A1 --- l_Diam Limit flag on Diam (1) 79- 83 F5.2 pc Diam [0.01/27] Diameter of the continuum source (2) 85- 85 A1 --- Code Association code between maser source and the continuum emission (G1) -------------------------------------------------------------------------------- Note (1): Upper limits given for the physical diameter of the corresponding continuum source due to our limited resolving power. Note (2): Diameter derived from the major axis "a" and the heliocentric distance of the associated maser. -------------------------------------------------------------------------------- Global notes: Note (G1): Code as follows: A = associated continuum emission is detected and classified as group A; B = continuum emission is found in the vicinity of the maser but with no evidence supporting physical relationship between maser and continuum source; N = Absence of continuum emission. -------------------------------------------------------------------------------- History: From electronic version of the journal 2017-Mar-18: Table 3 (correction of declination signs in Names) and Table 4 (corrections of some spot offsets) versions sent by the author 2022-Jun-10: Table 3, declination signs corrected (duplication of declination signs from Table 4) Acknowledgements: Bo Hu [Purple Mountain Observatory, Chinese Academy of Science, China]
(End) Prepared by [AAS], Emmanuelle Perret [CDS] 16-Mar-2017
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