Hα spectrum of VV Cephei - HD 208816 - SAO 19753 [M2epIa-Iab + B8:eV]
 |
VV Cephei is an eclipsing binary star system with a M2 and a B8 star The emission lines are caused by a disk around the B star, probable an accretion disk with material feeded by the supergiant M star. There is a campaign throug the next eclipse 2017 to 2019. More information about this: |
 |
| Telescope: Celestron C11 11" SC, f/10, d=280mm | Spectra with 2400 lines/mm, processed with BASS project | Download spectrum 1D FIT: |
| Spectrograph: Lhires III, 2400gr, slit 23u | Ha calibrated with internal Ar-Ne lamp, normalized flux | Download helioc.corr spec: vvCep_20151228.FIT |
| Camera: SBIG STT-8300M | Exposure time: 8 x 480s. | Download spectrum FIT (RAW): vvCep_8x8min_20151207.fit |
| Resolution: 0.0693 Å / pixel, resolving power = 18600 | Dark and Flat corrected, cropped, enlarged by factor 2 and stacked with PixInsight | Download BASS project bundle: vvCep_20151228.bun |
| Acquisition software: SbigControl, Guiding with DMKguider | Calibrated, RV-measure with HRV-MM2 | Download complete project(1.1MB): vvCep_20151228.zip |
| Date: 28. December 2015, 19:23 - 20:04 UT, JD 2457385.32 | ||
 |
||
 |
||
 |
||
  |
||
| Stellar data (Wikipedio.org): | ||
| Constellation: Cepheus, RA: 21h 56m 39.1s, Dec: +63° 37′ 32.0″ | ||
| v = 4.91 mag Mv = -6 | ||
| Distance: 4900 ly, 1500 pc | ||
| Mass: A ~ 25, B ~ 20 MΘ | ||
| Radius: A ~ 1600 - 1900, B ~10 RΘ | ||
| Luninosity: A ~ 200000-320000, B ~ 10000 LΘ | ||
| Surface Temperature: A: ~3800, B: ~25000 K | ||
