J/MNRAS/394/1875   IR colours of MASH planetary nebulae        (Phillips+, 2009)

The near- and far-infrared colours of MASH planetary nebulae. Phillips J.P., Zepeda-Garcia D. <Mon. Not. R. Astron. Soc., 394, 1875-1886 (2009)> =2009MNRAS.394.1875P 2009MNRAS.394.1875P
ADC_Keywords: Planetary nebulae ; Infrared sources ; Photometry, infrared Keywords: ISM: jets and outflows - planetary nebulae: general - infrared: ISM Abstract: We have analysed the near-infrared (NIR) and far-infrared (FIR) colours of MASH I and MASH II (the Macquarie/AAO/Strasbourg surveys, Cat. V/127) planetary nebulae (PNe), using data deriving from the Two-Micron All-Sky Survey and Infrared Astronomical Satellite. We were able to identify ∼5 per cent of the sources in the NIR, and a slightly larger fraction (∼12 per cent) in the FIR. It is concluded that whilst the NIR colours of these nebulae are consistent with those of less evolved (and higher surface brightness) PNe, their FIR colours are markedly different. This disparity is likely to arise as a result of an evolution in dust temperatures, in their line emission characteristics, and in the relative contributions of the 8.6 and 11.3um polycyclic aromatic hydrocarbon emission features. A rump of∼9 per cent of the detected sources have values log[F(25um)/F(60um)] which are lower than can be explained in terms of normal nebular evolution, however. If these are comparable in nature to the undetected PNe, then this would argue that ∼1 in 10 of MASH I and II nebulae may represent galactic H ii regions, Stromgren spheres, symbiotic nebulae or other unrelated categories of source. Description: We have investigated the fluxes of IRAS and 2MASS sources lying close to the MASH I and MASH II sources. This has involved correlating the positions of the MASH PNe with sources within 2MASS and IRAS point-source catalogues (PSCs). No identifications were found within the 2MASS extended source catalogue. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table1.dat 85 150 IRAS photometry for MASH I and MASH II sources table2.dat 97 60 2MASS photometry of MASH I and MASH II sources -------------------------------------------------------------------------------- See also: V/127 : MASH Catalogues of Planetary Nebulae (Parker+ 2006-2008) II/246 : 2MASS All-Sky Catalog of Point Sources (Cutri+ 2003) II/125 : IRAS catalogue of Point Sources, Version 2.0 (IPAC 1986) Byte-by-byte Description of file: table1.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 2 A2 --- --- [PN] 4- 15 A12 --- PNG PNG name (Gddd.d+dd.da) 17- 27 A11 --- IRAS IRAS name (HHMMm+DDMMA) 29- 32 A4 --- MASH MASH catalogue in which the sources appear (G1) 34- 45 A12 --- Name Nebular name 47 A1 --- TLP [TLP] PN status (G2) 49- 54 F6.2 Jy F12 Flux at 12um 56- 61 F6.2 Jy F25 Flux at 25um 63- 68 F6.2 Jy F60 Flux at 60um 70- 75 F6.2 Jy F100 Flux at 100um 77- 80 I4 --- Qual Quality flag in the 4 IRAS filters (3) 82- 85 F4.1 arcsec Sep Separation between the MASH and IR source position -------------------------------------------------------------------------------- Note (3): Reliability of the fluxes, where: 1 = upper limit 2 = moderate quality 3 = hight quality -------------------------------------------------------------------------------- Byte-by-byte Description of file: table2.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 2 A2 --- --- [PN] 4- 15 A12 --- PNG PNG name (Gddd.d+dd.da) 17- 32 A16 --- 2MASS 2MASS name (HHMMSSss+DDMMSSs) 35- 38 A4 --- MASH MASH catalogue in which the sources appear (G1) 40- 51 A12 --- Name Nebular name 53 A1 --- TLP [TLP] PN status (G2) 55- 58 F4.1 arcsec theta Harmonic mean size (3) 60- 64 F5.2 mag Jmag 2MASS J magnitude 66- 70 F5.3 mag e_Jmag rms uncertainty on Jmag 72- 76 F5.2 mag Hmag 2MASS H magnitude 78- 81 F4.2 mag e_Hmag rms uncertainty on Hmag 83- 87 F5.2 mag Ksmag 2MASS Ks magnitude 89- 93 F5.3 mag e_Ksmag rms uncertainty on Ksmag 94- 97 F4.1 arcsec Sep Separation between the MASH and 2MASS source position -------------------------------------------------------------------------------- Note (3): Harmonic mean size, θHARM=(θMax*θMin)0.5, where θMax and θMin are the maximum and minimum source sizes given in the MASH I and II catalogues -------------------------------------------------------------------------------- Global notes: Note (G1): MASH catalogue as follows: M I = Parker et al. 2006, Cat. V/127 M II = Miszalski et al. 2008, Cat. V/127 Note (G2): Flag of reliabilities of the PN: P = possible PN; L = likely PN; T = true PN -------------------------------------------------------------------------------- History: * 26-Oct-2009: From electronic version of the journal * 16-Nov-2009: 2MASS name corrected in table2 for PN G021.3+02.2; many other 2MASS names are not either the recommended 'truncated' J2000 position. * 15-Jun-2010: 3 2MASS names and 1 Name corrected in table2 - the names corrected are: 09572645-5357743 replaced by 09572645-5357074 18421140-0050317 replaced by 18421140+0050317 11281287-6121302 replaced by 11281287-6121030 - PHR1758-2756 replaced by PPA1757-2750
(End) Patricia Vannier [CDS] 01-Sep-2009
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