J/ApJS/161/240   High-ionization emission in metal-deficient BCDs (Thuan+, 2005)

High-ionization emission in metal-deficient blue compact dwarf galaxies. Thuan T.X., Izotov Y.I. <Astrophys. J. Suppl. Ser., 161, 240-270 (2005)> =2005ApJS..161..240T 2005ApJS..161..240T
ADC_Keywords: Abundances ; Equivalent widths ; H II regions Keywords: galaxies: abundances - galaxies: evolution - galaxies: irregular - galaxies: ISM Abstract: Primordial stars are expected to be very massive and hot, producing copious amounts of hard ionizing radiation. The best place to study hard ionizing radiation in the local universe is in very metal- deficient blue compact dwarf (BCD) galaxies. We have carried out a MMT spectroscopic search for [NeV] λ3426 (ionization potential of 7.1Ryd), [FeV] λ4227 (ionization potential of 4Ryd), and HeII λ4686 (ionization potential of 4Ryd) emission in a sample of 18 BCDs. We have added data from previous work and from the Data Release 3 of the Sloan Digital Sky Survey (Cat. II/259). In total, we have assembled a BCD high-ionization sample with [NeV] emission in four galaxies, [FeV] emission in 15 galaxies, and HeII emission in 465 galaxies. Description: We have obtained new high signal-to-noise ratio spectrophotometric observations for 26 HII regions in 18 BCDs and for one supergiant HII region in the spiral galaxy M101 with the 6.5m MMT on the nights of 2004 February 1920 and 2005 February 4. Three BCDs were observed by Izotov & Thuan (2004, Cat. J/ApJ/602/200) with the Kitt Peak 4m telescope and five others were selected from the DR3 of the SDSS (Abazajian et al. 2005, Cat. II/259). File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table1.dat 68 27 General parameters of galaxies table3.dat 84 767 Emission line intensities and equivalent width table4.dat 185 24 Ionic and total heavy element abundances table5.dat 84 334 Emission line intensities and equivalent widths in spectra obtained with other telescopes table6.dat 358 9 Ionic and total heavy element abundances in galaxies observed with other telescopes -------------------------------------------------------------------------------- See also: II/259 : The SDSS Photometric Catalog, Release 3 (Abazajian+ 2005) J/ApJ/511/639 : Abundances in blue compact galaxies (Izotov+, 1999) J/AZh/79/867 : Abundances of HII regions in blue galaxies (Holovatyy+, 2002) J/ApJ/602/200 : HII regions abundances in blue compact galaxies (Izotov+ 2004) J/A+A/419/469 : Abundances in the galaxy HS 0837+4717 (Pustilnik+, 2004) J/ApJS/161/240 : High-ionization emission in metal-deficient BCDs (Thuan+, 2005) J/A+A/448/955 : Abundances of emission galaxies in SDSS-DR3 (Izotov+, 2006) J/ApJ/708/1076 : The WHIQII survey: compact blue galaxies (Tollerud+, 2010) Byte-by-byte Description of file: table1.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 12 A12 --- Name Galaxy name 13 A1 --- m_Name [AEW] Multiplicity flag on Name 15 A1 --- n_Name [ABC] Flag on Name (1) 17- 18 I2 h RAh Hour of Right Ascension (J2000.0) 20- 21 I2 min RAm Minute of Right Ascension (J2000.0) 23- 26 F4.1 s RAs Second of Right Ascension (J2000.0) 28 A1 --- DE- Sign of the Declination (J2000.0) 29- 30 I2 deg DEd Degree of Declination (J2000.0) 32- 33 I2 arcmin DEm Arcminute of Declination (J2000.0) 35- 36 I2 arcsec DEs Arcsecond of Declination (J2000.0) 38- 41 F4.1 mag pgmag Apparent photographic magnitude 43- 49 F7.5 --- z Redshift 51- 55 F5.1 mag pgMAG Absolute photographic magnitude 57- 68 A12 --- OName Other name -------------------------------------------------------------------------------- Note (1): Flag on Name, defined as follows: A = Galaxies observed with the MMT B = Galaxies observed with the 4m KPNO telescope with detected [FeV] λ4227 emission C = SDSS galaxies with detected [FeV] λ4227 emission -------------------------------------------------------------------------------- Byte-by-byte Description of file: table3.dat table5.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 12 A12 --- Name Galaxy name 13- 14 A2 --- m_Name Multiplicity flag on Name 16- 20 F5.3 --- CHb Hβ extinction coefficient 22- 27 F6.3 10-17W/m2 FHb Observed Hβ flux in units of 10-14 erg/s/cm2 28- 31 F4.2 0.1nm EWabs Hydrogen absorption equivalent width 33- 36 I4 0.1nm lambda Wavelength (Å) 38- 51 A14 --- Ion Ion designation 53- 58 F6.2 --- F/FHb Observed flux relative to Hβ 60- 64 F5.2 --- e_F/FHb Statistical error in F/FHb 66- 71 F6.2 --- I/IHb Corrected flux relative to Hβ 73- 77 F5.2 --- e_I/IHb Statistical error in I/IHb 79- 84 F6.1 0.1nm EW Equivalent width of Ion -------------------------------------------------------------------------------- Byte-by-byte Description of file: table4.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 12 A12 --- Name Galaxy name 15- 16 A2 --- m_Name Multiplicity index on Name 18- 22 I5 K Te(OIII) OIII electron temperature 24- 27 I4 K e_Te(OIII) Error in Te(OIII) 29- 33 I5 K Te(OII) OII electron temperature 35- 37 I3 K e_Te(OII) Error in Te(OII) 39- 43 F5.3 10-4 O+/H+ O+/H+ abundance ratio 45- 49 F5.3 10-4 e_O+/H+ Error in O+/H+ 51- 55 F5.3 10-4 O++/H+ O++/H+ abundance ratio 57- 61 F5.3 10-4 e_O++/H+ Error in O++/H+ 63- 67 F5.3 10-6 O+++/H+ ? O+++/H+ abundance ratio 69- 73 F5.3 10-6 e_O+++/H+ ? Error in O+++/H+ 75- 79 F5.3 10-4 O/H O/H abundance ratio 81- 85 F5.3 10-4 e_O/H Error in O/H 87- 91 F5.3 [---] 12+log(O/H) Oxygen abundance 93- 97 F5.3 [---] e_12+log(O/H) Error in log(O/H) 99-103 F5.3 10-5 Ne++/H+ Ne++/H+ abundance ratio 105-109 F5.3 10-5 e_Ne++/H+ Error in Ne++/H+ 111-115 F5.3 --- ICF(Ne) ? Ionization correction factor 117-122 F6.3 [---] log(Ne/O) log(Ne/O) abundance ratio 124-128 F5.3 [---] e_log(Ne/O) Error in log(Ne/O) 130-134 F5.3 10-6 Fe++/H+1 ? Fe++(4658)/H+ abundance ratio 136-140 F5.3 10-6 e_Fe++/H+1 ? Error in Fe++/H+1 142-146 F5.3 10-6 Fe++/H+2 ? Fe++(4988)/H+ abundance ratio 148-152 F5.3 10-6 e_Fe++/H+2 ? Error in Fe++/H+2 154-159 F6.3 --- ICF(Fe) ? Ionization correction factor 161-166 F6.3 [---] log(Fe/O)1 ? log(Fe(4658)/O) abundance ratio 168-172 F5.3 [---] e_log(Fe/O)1 ? Error in log(Fe/O)1 174-179 F6.3 [---] log(Fe/O)2 ? log(Fe(4988)/O) abundance ratio 181-185 F5.3 [---] e_log(Fe/O)2 ? Error in log(Fe/O)2 -------------------------------------------------------------------------------- Byte-by-byte Description of file: table6.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 12 A12 --- Name Galaxy name 15- 16 A2 --- m_Name Multiplicity index on Name 18- 22 I5 K TeOIII OIII electron temperature 24- 27 I4 K e_TeOIII Error in TeOIII 29- 33 I5 K TeOII OII electron temperature 35- 37 I3 K e_TeOII Error in TeOII 39- 43 I5 K TeSIII SIII electron temperature 45- 47 I3 K e_TeSIII Error in TeSIII 49- 52 I4 cm-3 NeSII SII electron number density 54- 56 I3 cm-3 e_NeSII Error in NeSII 58- 62 F5.3 10-4 O+/H+ O+/H+ abundance ratio 64- 68 F5.3 10-4 e_O+/H+ Error in O+/H+ 70- 74 F5.3 10-4 O++/H+ O++/H+ abundance ratio 76- 80 F5.3 10-4 e_O++/H+ Error in O++/H+ 82- 86 F5.3 10-6 O+++/H+ O+++/H+ abundance ratio 88- 92 F5.3 10-6 e_O+++/H+ Error in O+++/H+ 94- 98 F5.3 10-4 O/H O/H abundance ratio 100-104 F5.3 10-4 e_O/H Error in O/H 106-110 F5.3 [---] 12+log(O/H) Oxygen abundance 112-116 F5.3 [---] e_12+log(O/H) Error in 12 + log(O/H) 118-122 F5.3 10-6 N+/H+ N+/H+ abundance ratio 124-128 F5.3 10-6 e_N+/H+ Error in N+/H+ 130-134 F5.3 --- ICF(N) Ionization correction factor 136-141 F6.3 [---] log(N/O) log(N/O) abundance ratio 143-147 F5.3 [---] e_log(N/O) Error in log(N/O) 149-153 F5.3 10-5 Ne++/H+ Ne++/H+ abundance ratio 155-159 F5.3 10-5 e_Ne++/H+ Error in Ne++/H+ 161-165 F5.3 --- ICF(Ne) Ionization correction factor 167-172 F6.3 [---] log(Ne/O) log(Ne/O) abundance ratio 174-178 F5.3 [---] e_log(Ne/O) Error in log(Ne/O) 180-184 F5.3 10-6 S+/H+ S+/H+ abundance ratio 186-190 F5.3 10-6 e_S+/H+ Error in S+/H+ 192-196 F5.3 10-6 S++/H+ S++/H+ abundance ratio 198-202 F5.3 10-6 e_S++/H+ Error in S++/H+ 204-208 F5.3 --- ICF(S) Ionization correction factor 210-215 F6.3 [---] log(S/O) log(S/O) abundance ratio 217-221 F5.3 [---] e_log(S/O) Error in log(S/O) 223-227 F5.3 10-8 Cl++/H+ ? Cl++/H+ abundance ratio 229-233 F5.3 10-8 e_Cl++/H+ ? Error in Cl++/H+ 236-240 F5.3 --- ICF(Cl) ? Ionization correction factor 242-247 F6.3 [---] log(Cl/O) ? log(Cl/O) abundance ratio 249-253 F5.3 [---] e_log(Cl/O) ? Error in log(Cl/O) 259-263 F5.3 10-7 Ar++/H+ Ar++/H+ abundance ratio 265-269 F5.3 10-7 e_Ar++/H+ Error in Ar++/H+ (1e7) 272-276 F5.3 10-7 Ar+++/H+ ? Ar+++/H+ abundance ratio 278-282 F5.3 10-7 e_Ar+++/H+ ? Error in Ar+++/H+ 285-289 F5.3 --- ICF(Ar) Ionization correction factor 291-296 F6.3 [---] log(Ar/O) log(Ar/O) abundance ratio 298-302 F5.3 [---] e_log(Ar/O) Error in log(Ar/O) 304-308 F5.3 10-6 Fe++/H+1 ? Fe++(4658)/H+ abundance ratio 310-314 F5.3 10-6 e_Fe++/H+1 ? Error in Fe++/H+1 316-320 F5.3 10-6 Fe++/H+2 ? Fe++(4988)/H+ abundance ratio 322-326 F5.3 10-6 e_Fe++/H+2 ? Error in Fe++/H+2 328-332 F5.3 --- ICF(Fe) ? Ionization correction factor 334-339 F6.3 [---] log(Fe/O)1 ? log(Fe(4658)/O) abundance ratio 341-345 F5.3 [---] e_log(Fe/O)1 ? Error in log(Fe/O)1 347-352 F6.3 [---] log(Fe/O)2 ? log(Fe(4988)/O) 354-358 F5.3 [---] e_log(Fe/O)2 ? Error in log(Fe/O)2 -------------------------------------------------------------------------------- History: From electronic version of the journal
(End) Greg Schwarz [AAS], Marianne Brouty [CDS] 13-Jun-2006
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