Web19 lug 2016 · HFG1 (136+5°1) is a large, low-surface-brightness planetary nebula that was discovered by Heckathorn, Fesen, and Gull (Astrpn. Astronphys. , 114, 414, 1982). in the … Web14 mag 2007 · Planetary Nebula HFG 1 - posted in Experienced Deep Sky Imaging: This was a real challenge from light-polluted skies. ... HFG1 (PK 136+05, PN G136.3+05.5) is about 14th magnitude and 8.5 arc minutes in diameter. It was discovered in the Milky Way Emission Line Study in 1982.
HFG 1 — AAPOD2.COM
Web16 mar 2009 · A deep wide-field image in the light of the Halpha+[N II] emission lines, of the planetary nebula HFG1 which surrounds the precataclysmic binary system V664 Cas, has revealed a tail of emission at least 20' long, at a position angle of 316deg. Evidence is presented which suggests that this is an ~10^5 y old trail of shocked material, left behind … WebHFG1 (PK 136+05) and Abell 6 (PK 136+4.1) form the most original planetary nebula duo to be imaged. They are located in Cassiopea. HFG1 was discovered in the Milky Way … pef retro longevity payments 2021
HFG1: A Planetary Nebula with a Close-Binary Nucleus
Web3 ago 2024 · Abell 6 + HFG1 - posted in Experienced Deep Sky Imaging: Abell 6 (PK 136+04 1 and others) at the center of the image, is a planetary nebula located approximately 3,154 light-years away. HFG1 (PK 136+05 1 and others) at the top left, is a planetary nebula located approximately 2,308 light-years away. Both of these are … Web5 ago 2024 · Page 1 of 2 - Heckathorn-Fesen-Gull 1 (HFG1) - 82 hours integration time with TS ONTC 10in f4 - posted in Experienced Deep Sky Imaging: Heckathorn-Fesen-Gull 1 (HFG1, PK136+05) is a very old (~100,000 year old) and extremely faint planetary nebula in the constellation Cassiopeia. It was discovered in deep OIII images by Heckathorn, … Web19 lug 2016 · HFG1 (136+5°1) is a large, low-surface-brightness planetary nebula that was discovered by Heckathorn, Fesen, and Gull (Astrpn. Astronphys. , 114, 414, 1982). in the autumn of 1986, photoelectric photometry by A.D.G. and H.E.B. showed that the 14th-mag central star of HFG1 is a large-amplitude variable. pef promotion percentage