NN Ser spectrum during total eclipse
This chart represents the spectrum of the cool dwarf star in the variable stellar system NN Ser . The 5 min exposure was obtained during the total phase of the eclipse, when the magnitude of the system was V = 23.0. Several TiO bands are clearly visible in this slightly smoothed tracing. A few deep and narrow "absorption" features are residuals from sky subtraction. The original resolution is 0.55 nm/pix. A spectral type of M6 or later is deduced for NN Ser . The spectrum of a more nearby (and hence much brighter) M6.5 dwarf star (temperature approx. 2600 degrees) is shown below for comparison.
Źródło:ESO
O zdjęciu
Identyfikator: | eso9936d |
Typ: | Obserwacje |
Data publikacji: | 20 lipca 1999 |
Powiązane komunikaty: | eso9936 |
Rozmiar: | 960 x 723 px |
O obiekcie
Nazwa: | NN Serpentis, Spectrum |
Typ: | Milky Way : Star : Grouping : Binary |
Odległość: | 1500 lat świetlnych |
Kategoria: | Stars |
Kolory i filtry
Pasmo | Teleskop |
---|---|
Podczerwony Near-IR | Very Large Telescope FORS1 |
Optyczny | Very Large Telescope FORS1 |