J/A+A/561/A119    Spectra of stars and planetary nebulae    (Moni Bidin+, 2014)

Investigating potential planetary nebula/cluster pairs. Moni Bidin C., Majaess D., Bonatto C., Mauro F., Turner D., Geisler D., Chene A.-N., Gormaz-Matamala A.C., Borissova J., Kurtev R.G., Minniti D., Carraro G., Gieren W. <Astron. Astrophys. 561, A119 (2014)> =2014A&A...561A.119M 2014A&A...561A.119M
ADC_Keywords: Clusters, open ; Planetary nebulae ; Radial velocities Keywords: planetary nebulae: general - open clusters: and associations: general Abstract: Fundamental parameters characterizing the end-state of intermediate-mass stars may be constrained by discovering planetary nebulae (PNe) in open clusters (OCs). Cluster membership may be exploited to establish the distance, luminosity, age, and physical size for PNe, and the intrinsic luminosity and mass of its central star. Four potential PN-OC associations were investigated to assess the cluster membership for the PNe. Radial velocities were measured from intermediate-resolution optical spectra, complemented with previous estimates in the literature.When the radial velocity study supported the PN/OC association, we analyzed whether other parameters (e.g., age, distance, reddening, central star brightness) were consistent with this conclusion. Description: The spectra were collected on 2012-04-13 with the B&C spectrograph at the focus of the 2.5m du Pont telescope at the Las Campanas observatory. The 1200 line/mm grating was used at the second order, with a grating angle of 56.12°, thus collecting data in the spectral interval 596-666nm. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file stars.dat 83 33 List of studied stars sp/* . 33 Individual spectrum (596-666nm) -------------------------------------------------------------------------------- See also: V/84 : Strasbourg-ESO Catalogue of Galactic Planetary Nebulae (Acker+, 1992 Byte-by-byte Description of file: stars.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 2 I2 h RAh Simbad Right ascension (J2000) 4- 5 I2 min RAm Simbad Right ascension (J2000) 7- 11 F5.2 s RAs Simbad Right ascension (J2000) 13 A1 --- DE- Simbad Declination sign (J2000) 14- 15 I2 deg DEd Simbad Declination (J2000) 17- 18 I2 arcmin DEm Simbad Declination (J2000) 20- 23 F4.1 arcsec DEs Simbad Declination (J2000) 25- 47 A23 --- Name Star name 49- 59 A11 --- FileName Name of the file with spectrum in subdirectory sp 61- 83 A23 --- SName Simbad name -------------------------------------------------------------------------------- Byte-by-byte Description of file: sp/* -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 7 F7.2 0.1nm lambda [5959/6656] Wavelength (Å) 9- 24 F16.10 --- Flux Normalized flux -------------------------------------------------------------------------------- Acknowledgements: Christian Moni Bidin, chr.moni.bidin(at)gmail.com
(End) Christian Moni Bidin [UCN, Chile], Patricia Vannier [CDS] 20-Dec-2013
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