December 28, 2018
NGC 1491 (Dec. 2018)
This is 21x1800" with the SXVF-H9 through the 6nm Astronomik H-alpha filter and Synta-ONTC 8" f/4.95 Newt. The brighter star in the center driving the hydrogen emission is 11.2-magnitude BD +50 886, classified as O5 or O4. Source. The nebula is probably over 10,000 light years away. I was able to catch two nights on this nebula. The first night was somewhat less transparent, but the data seemed good. The second night had excellent transparency.
Labels:
1491,
SXVF-H9,
Synta-ONTC Newtonian
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