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J/A+A/512/A83    Velocities of interstellar lines in Sco-Cen   (Poeppel+, 2010)

The interstellar medium surrounding the Scorpius-Centaurus association revisited. Poeppel W.G.L., Bajaja E., Arnal E.M., Morras R. <Astron. Astrophys., 512, A83-83 (2010)> =2010A&A...512A..83P
ADC_Keywords: Associations, stellar ; Interstellar medium ; Radial velocities Keywords: open clusters and associations: individual: Sco-Cen association - open clusters and associations: individual: Gould Belt - ISM: clouds Abstract: We want to make a large-scale study of the morphology, kinematics, and origin of the HI, which surrounds the Sco-Cen association. We combine our high-sensitivity southern HI survey with the Leiden/Dwingeloo Survey, considering l=240°-400°, b=-60° to +60°, and radial velocities of V=-41.8 to +40.8km/s. We point out the main HI branches surrounding the association and derive their kinematics. Kinematical HI-maps were compared with spatial maps of interstellar (IS) NaI from the literature. Upper limits for distances d were derived from optical IS absorption components from the literature. Models of expanding spherical HI shells were fitted around each stellar subgroup. Description: In this paper we are using our new high-sensitivity southern 21-cm line survey (see Arnal et al., 2000, ASP Conf. Ser., 218, 401), combined with the Leiden/Dwingeloo Survey of Galactic Neutral Hydrogen (Hartmann & Burton, 1997, Atlas of Galactic Neutral Hydrogen (Cambridge Univ. Press)). File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file tablea1.dat 97 426 Data base of optical interstellar absorption lines refs.dat 70 32 References
See also: J/ApJS/93/211 : IUE survey of HI Lyα absorption. I. (Diplas+ 1994) J/AJ/124/404 : Upper Scorpius OB assoc. Lithium survey. II. (Preibisch, 2002) Byte-by-byte Description of file: tablea1.dat
Bytes Format Units Label Explanations
1- 2 I2 --- Panel [1/19] Panel number 4- 14 A11 --- Name Star name 16- 20 F5.1 deg GLON [98/398] Galactic longitude 23- 27 F5.1 deg GLAT Galactic latitude 29- 31 I3 pc Dist Heliocentric star distance 32 A1 --- q_Dist [?hd] Note on the distance accuracy (1) 34- 38 A5 --- IS Observed interstellar species 40- 44 F5.1 km/s V1 ? Radial velocity of IS component 46- 50 F5.1 km/s V2 ? Radial velocity of IS component 52- 56 F5.1 km/s V3 ? Radial velocity of IS component 58- 62 F5.1 km/s V4 ? Radial velocity of IS component 64- 67 F4.1 km/s V5 ? Radial velocity of IS component 69- 73 F5.1 km/s V6 ? Radial velocity of IS component 75- 78 F4.2 km/s dV ? Velocity resolution 80- 84 A5 --- Ref Reference number, in refs.dat file 86- 97 A12 --- Com Comments (2)
Note (1): Note on distance as follows: h = Hipparcos-value with an uncertainty smaller than 20% d = Hipparcos-value with an uncertainty larger than 20% ? = uncertainty flag Note (2): the footnote (1) indicates a clear signal read off from the published plot although not mentioned by the authors
Byte-by-byte Description of file: refs.dat
Bytes Format Units Label Explanations
1- 2 I2 --- Ref Reference code 4- 22 A19 --- BibCode BibCode 24- 42 A19 --- Aut Author's name 44- 70 A27 --- Com Comments
History: From electronic version of the journal
(End) Patricia Vannier [CDS] 07-Jul-2010
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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