Results - We are eager for every contribution

Here we present some representative and definite results to show expected campaign spectra.

 


Two exposures from Berthold Stober / Glan-Münchweiler

Time difference about 2 days. Strong line variations are present. They represent a turbulent wind (clumps) of the WR component.

Exposure from Berthold Stober / Glan-Münchweiler

C14 (D=355 mm, f=3550mm), Slit spektrograph (Littrow), exposure time 2 hours.

Exposure from Berthold Stober / Glan-Münchweiler

C14 (D=355 mm, f=3550mm), Slit spektrograph (Littrow)

Exposure from Berthold Stober / Glan-Münchweiler

C14 (D=355 mm, f=3550mm), Slit spektrograph (Littrow)

Exposure from Lothar Schanne / Voelklingen

C14, Lhires with 2400 g/mm grating, Nova 1602E im 2x2 binning (0,27 A/Pix), 300s. Calibration with Neon lamp. Data reduction with IRIS and VSpec. FWHM of slit image 0,84A at 50 um slit width.

Exposure from Lothar Schanne / Voelklingen

C14, Lhires with 2400 g/mm grating, Nova 1602E im 2x2 binning (0,27 A/Pix), 300s. Calibration with Neon lamp. Data reduction with IRIS and VSpec. FWHM of slit image 0,84A at 50 um slit width.

Exposure from Berthold Stober / Glan-Münchweiler

C14 (D=355 mm, f=3550mm), Slit spektrograph (Littrow)

Exposure from Berthold Stober / Glan-Münchweiler

C14 (D=355 mm, f=3550mm), Slit spektrograph (Littrow)