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Variable star in the constellation Pegasus
LL Pegasi (AFGL 3068) is a Mira variable star surrounded by a pinwheel-shaped nebula, IRAS 23166+1655, thought to be a preplanetary nebula. It is a binary
LL_Pegasi
Spiral with constant distance from itself
made by a Catherine's wheel) are Archimedean. For instance, the star LL Pegasi shows an approximate Archimedean spiral in the dust clouds surrounding
Archimedean_spiral
similar to Betelgeuse. RT Carinae 1,090 L/Teff UU Persei 1,079+9 −8 L/Teff LL Pegasi 1,070 L/Teff HD 126577 1,066+9 −32 L/Teff HaroChavira 1 1,058 L/Teff EV
List_of_largest_stars
Type of variable star
for composite grains in an AGB outflow. MgS in the extreme carbon star LL Pegasi". Astronomy & Astrophysics. 544: L18. arXiv:1207.1606. Bibcode:2012A&A
Mira_variable
Nebula IRAS 04395+3601 1975 3,600 ± 700 IRAS 13208-6020 IRAS 20068+4051 LL Pegasi IRAS 23166+1655 1975 4,000 M1-92 IRAS 19343+2926 1946 8,000 IRAS 19024+0044
List of protoplanetary nebulae
List_of_protoplanetary_nebulae
Star whose atmosphere contains more carbon than oxygen
researcher of carbon stars La Superba, one of the more well known carbon stars LL Pegasi, which has so much soot in it that it has created a spiral trail of smoke
Carbon_star
Distance (light years) Notes S Cassiopeiae 1,800 S3,4–S5,8 3,100±300 LL Pegasi 1,800 C 4,200 RW Leonis Minoris 1,800 C4,3 1,053 V Coronae Borealis 1
List_of_coolest_stars
Variable star in the constellation Pegasus
φ Pegasi, Latinised as Phi Pegasi, is a solitary, reddish hued star in the northern constellation of Pegasus. With an apparent visual magnitude of around
Phi_Pegasi
Star in the constellation Pegasus
σ Pegasi, Latinised as Sigma Pegasi, is a binary star system in the northern constellation of Pegasus. With a combined apparent visual magnitude of 5
Sigma_Pegasi
Star in the constellation Pegasus
Exoplanets 51 Pegasi b (Dimidium) AT2021ueyLb BD+05 4868Ab BD+14 4559 b (Pirx) HAT-P-8b HD 209458 b HD 210702 b HD 219828 b HR 8799 b c d e V391 Pegasi b WASP-10b
Gliese_880
White dwarf in the constellation Pegasus
Exoplanets 51 Pegasi b (Dimidium) AT2021ueyLb BD+05 4868Ab BD+14 4559 b (Pirx) HAT-P-8b HD 209458 b HD 210702 b HD 219828 b HR 8799 b c d e V391 Pegasi b WASP-10b
WD_2317+1830
Shock wave caused by blowing stellar wind
BZ Camelopardalis, V341 Ara, SY Cancri, ASASSN-V J205457.73+515731.9, LS Pegasi, and FY Vulpeculae. Recent discoveries were partly made with the help of
Bow_shock
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