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J/A+A/416/515         Long slit spectroscopy of HII regions     (Marquez+, 2004)

Starbursts in barred spiral galaxies. VI. HI observations and the K-band Tully-Fisher relation. Davoust E., Contini T. <Astron. Astrophys. 416, 515 (2004)> =2004A&A...416..515D
ADC_Keywords: Galaxies, Markarian ; Galaxies, IR ; H I data ; Radial velocities Keywords: galaxies: starburst - galaxies: active - galaxies: evolution - galaxies: ISM - galaxies: kinematics and dynamics - radio lines: galaxies Abstract: This paper reports a study of the effect of a bar on the neutral hydrogen (HI) content of starburst and Seyfert galaxies. We also make comparisons with a sample of "normal" galaxies and investigate how well starburst and Seyfert galaxies follow the fundamental scaling Tully-Fisher (TF) relation defined for normal galaxies. 111 Markarian (Mrk) IRAS galaxies were observed with the Nancay radiotelescope, and HI data were obtained for 80 galaxies, of which 64 are new detections. We determined the (20 and 50%) linewidths, the maximum velocity of rotation and total HI flux for each galaxy. These measurements are complemented by data from the literature to form a sample of Mrk IRAS (74% starburst, 23% Seyfert and 3% unknown) galaxies containing 105 unbarred and 113 barred ones. Barred galaxies have lower total and bias-corrected HI masses than unbarred galaxies, and this is true for both Mrk IRAS and normal galaxies. This robust result suggests that bars funnel the HI gas toward the center of the galaxy where it becomes molecular before forming new stars. The Mrk IRAS galaxies have higher bias-corrected HI masses than normal galaxies. They also show significant departures from the TF relation, both in the B and K bands. The most deviant points from the TF relation tend to have a strong far-infrared luminosity and a low oxygen abundance. These results suggest that a fraction of our Mrk IRAS galaxies are still in the process of formation, and that their neutral HI gas, partly of external origin, has not yet reached a stationary state. Description: The observations were obtained at the large decimetric radiotelescope of Nancay Observatory. Three runs (a total of 281h) were allocated for the barred subsample in 1993-94, and six runs (214h) for the unbarred subsample in 1996-99. We observed a total of 111 galaxies, and detected 80 (+ one companion), of which 64 are new detections. File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file table4.dat 46 17 Galaxies with the strongest deviations from the K-band TF relation table5.dat 60 106 HI data for Markarian galaxies observed at the Nancay Radiotelescope table6.dat 86 218 Integrated quantities for the Mrk IRAS galaxies
See also: J/A+AS/130/285 : Sample of starburst nucleus galaxies (Contini+ 1998) Byte-by-byte Description of file: table4.dat
Bytes Format Units Label Explanations
1 A1 --- Type [BU] B: Barred Galaxies, U: Unbarred Galaxies 3- 6 I4 --- Mrk Galaxy name 8- 10 A3 --- SpType spectral type 12- 15 F4.2 --- O/H ? Oxygen abundance 17- 21 F5.2 [solLum] logFIR log of far infrared luminosity (1) 23- 27 F5.2 --- DMHI Excess of HI mass (1) 29- 34 F6.3 [km/s] DlogVm Difference between log of observed and expected Vm (maximum velocity of rotation) 36- 46 A11 --- Envir Environment
Note (1): Means values: Barred Galaxies : logFIR = 10.21, DMHI = 0.30 Unbarred Galaxies : logFIR = 10.13, DMHI = 0.33
Byte-by-byte Description of file: table5.dat
Bytes Format Units Label Explanations
1- 8 A8 --- Name Galaxy name (Mrk or UGC) 10- 13 F4.1 --- TType ? Morphological type 16- 17 I2 deg Incl ? Inclination 21- 25 I5 km/s HRV Heliocentric radial velocity 26 A1 --- r_HRV [)] ) when from LEDA 28- 29 I2 km/s e_HRV ? Uncertainty on heliocentric radial velocity 31- 34 F4.1 mJy rms rms noise 36- 39 F4.1 --- SNR ? Signal-to-noise ratio 41- 43 I3 km/s W20 ? Linewidth at 20% of maximum intensity 45- 47 I3 km/s W50 Linewidth at 50% of maximum intensity 48 A1 --- u_W50 [)] ) when W50 estimated (1) 50 A1 --- l_FHI Upper limit on HI flux density 51- 55 F5.2 Jy.km/s FHI HI flux density 57- 60 F4.2 Jy.km/s e_FHI ? uncertainty on HI flux density
Note (1): When no line was detected, the listed W50 was estimated from the Tully-Fisher relation and is given in brackets.
Byte-by-byte Description of file: table6.dat
Bytes Format Units Label Explanations
1- 4 I4 --- Mrk Galaxy name 6- 7 A2 --- Bar bar/no bar 9- 11 A3 --- SpType spectral type 13- 16 F4.1 --- MType Morphological type 18- 21 F4.1 deg Incl Inclination 23- 27 F5.3 [0.1arcmin] logdc log of isophotal diameter 29- 33 F5.3 [0.1arcmin] e_logdc Uncertainty on log of isophotal diameter 35- 39 F5.3 [km/s] logVm log of maximum velocity of rotation 41- 45 F5.3 [km/s] e_logVm Uncertainty on log of maximum velocity of rotation 47- 51 F5.1 Mpc Dist Distance 53- 57 F5.2 mag Kmag K-band magnitude 59- 62 F4.2 --- O/H Oxygen abundance 64- 68 F5.2 [solMass] logMHI log of total HI mass 70- 73 F4.2 [solMass] e_logMHI Uncertainty on log of HI mass 75- 79 F5.2 [solLum] logFIR log of far infrared luminosity 81- 86 F6.2 mag BMAG Absolute B magnitude
Acknowledgements: Emmanuel Davoust References: Contini et al., Paper I 1995A&A...303..440C Contini et al., Paper II 1997A&A...324...41C Contini et al., Paper III 1998A&AS..130..285C, Cat. J/A+AS/130/285 Considere et al., Paper IV 2000A&A...356...89C Chapelon et al., Paper V 1999A&A...345...81C
(End) Patricia Bauer [CDS] 12-Mar-2004
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

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