J/ApJS/131/47   Gas-rich dwarfs from the POSS-II. III.       (Eder+, 2000)

Gas-rich dwarfs from the PSS-II. III. H I profiles and dynamical masses. Eder J.A., Schombert J.M. <Astrophys. J. Suppl. Ser. 131, 47 (2000)> =2000ApJS..131...47E 2000ApJS..131...47E
ADC_Keywords: Galaxies, radio ; H I data ; Radio lines Keywords: galaxies: dwarf - galaxies: fundamental parameters - galaxies: ISM - galaxies: kinematics and dynamics - radio lines: galaxies Abstract: We present Arecibo neutral hydrogen data on a sample of optically selected dwarf galaxies. The sample ranges in H I mass from 106 to 5x109M, with a mean of 7.9x108M. Using estimated H I radii, the H I surface densities range from 0.6 to 20M/pc2, all well below the critical threshold for star formation (Kennicutt, 1998ApJ...498..541K 1998ApJ...498..541K). MHI/L values of the LSB dwarfs range from 0.3 to 12 with a mean value of 2.0. Dynamical masses, calculated from the H I profile widths, range from 108 to 1011M. There is a strong correlation between optical luminosity and dynamical mass for LSB dwarfs implying that the dark matter (whether baryonic or nonbaryonic) follows the detectable baryonic matter. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table1.dat 71 389 LSB Dwarf Galaxy Sample table2.dat 41 64 Optical and Mass Parameters -------------------------------------------------------------------------------- Byte-by-byte Description of file: table1.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 7 A7 --- ESDO Object identification from Schombert et al., 1997ApJS..111..233S 1997ApJS..111..233S, (1) 10- 11 I2 h RAh Right Ascension (B1950) (2) 13- 14 I2 min RAm Right Ascension (B1950) (2) 16- 19 F4.1 s RAs Right Ascension (B1950) (2) 22- 23 I2 deg DEd Declination (B1950) (2) 25- 26 I2 arcmin DEm Declination (B1950) (2) 28- 29 I2 arcsec DEs Declination (B1950) (2) 32- 36 I5 km/s HVel ? The H I line Heliocentric velocity measured at the profile midpoint 39- 43 I5 km/s Vel ? The H I line Local Group velocity (3) 46- 48 I3 km/s VWidth ? Velocity width 50 A1 --- Shape [DS] Profile shape (4) 51 A1 --- u_Shape [:] Indicates an uncertain classification 55- 59 I5 mJy.km/s Flux ? Observed integrated 21cm H I line flux 62- 66 F5.2 [solMass] LogHMass ? The log of the H I mass in solar units 69 I1 --- RunCode Observing run number data was taken from (5) -------------------------------------------------------------------------------- Note (1): Based on the PSS-II field number and a running number for the dwarfs found on that field. Note (2): Measured off the PSS-II plates. Accurate to 15 arcsecs. Note (3): Velocity calculated according to the precepts of de Vaucouleurs, de Vaucouleurs, and Corwin (1976, Cat. VII/112). Note (4): Profile shape S = single-horned profile D = double-horned profile Note (5): Observing runs: 1 = Sample 1 observed in 1986 2 = Sample 2 observed in 1992 and 1993 3 = Sample 3 observed in 1992 and 1993 -------------------------------------------------------------------------------- Byte-by-byte Description of file: table2.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 7 A7 --- ESDO Object identification (1) 10- 13 F4.1 arcsec Rad The B band 25 mag isophotal radius 16- 19 F4.2 --- b/a Axial ratio (b/a) 22- 26 F5.1 mag IMag Absolute I band magnitude 29- 33 F5.2 [solMass/pc2] logSdens Log of the H I surface density 36- 40 F5.2 [solMass] LogMass Log of the dynamical mass -------------------------------------------------------------------------------- Note (1): Based on the PSS-II field number and a running number for the dwarfs found on that field. -------------------------------------------------------------------------------- History: * 24-Jan-2001: Prepared by Greg Schwarz [AAS] * 12-Mar-2001: Corrected coordinates of the 4 sources 500-1, 575-8, 646-1, 721-9 according to Paper I (in agreement with Jim Schombert) References: Schombert et al., Paper I 1997ApJS..111..233S 1997ApJS..111..233S Pildis et al., Paper II 1997ApJ...481..157P 1997ApJ...481..157P
(End) Greg Schwarz [AAS], Patricia Bauer [CDS] 12-Mar-2001
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