V380 Ori emission line spectrum : J/A+AS/136/95

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Authors : Rossi C. orcid , Errico L., Friedjung M. (hide) , Errico L., Friedjung M. et..al

VizieR DOI :
Bibcode : 1999A&AS..136...95R (ADS) (Simbad) (Objects)
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CDS Keywords : Stars, Be; Spectroscopy; Equivalent widths
UAT : Be stars, Spectroscopy, Line intensities

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Inserted into VizieR : 07-Apr-1999
Last modification : 12-Apr-1999

On the nature of the Herbig Be star V380 Orionis (1999)

Keywords : stars emission line, Be - stars: individual: V380 Ori - stars: pre-main sequence - infrared: stars - ultraviolet: stars

Abstract:Table 3 presents the emission line spectrum of V380 Ori in the optical region observed at OHP in January 1995 with a mean resolution of 10000. For the line blends the wavelength and flux (not reddening corrected) of each contributor are given. For the P-Cygni profiles the equivalent widths of the absorption component are also reported. We estimate an error of less than 10% for the strongest lines, 10% to 40% for the weakest lines. ...(more)
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Table 3 presents the emission line spectrum of V380 Ori in the optical region observed at OHP in January 1995 with a mean resolution of 10000. For the line blends the wavelength and flux (not reddening corrected) of each contributor are given. For the P-Cygni profiles the equivalent widths of the absorption component are also reported. We estimate an error of less than 10% for the strongest lines, 10% to 40% for the weakest lines.
Corinne Rossi 

                


                

                    

                


                

                    

                


                

                    
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