LL Andromedae

LL Andromedae (often abbreviated to LL And) is a dwarf nova in the constellation Andromeda, discovered during an outburst in 1979. Its typical apparent visual magnitude is 19.4, but undergoes outbursts events when can reach a peak magnitude of 14.3.[2] Since this magnitude is reached during the most powerful outbursts, while less bright outbursts can occur, it is classified as a SU Ursae Majoris variable.[1]

LL Andromedae
Observation data
Epoch J2000      Equinox J2000
Constellation Andromeda
Right ascension  00h 41m 51.46s[1]
Declination +26° 31′ 21.3″[1]
Apparent magnitude (V) 14.3 – 19.4 variable[2]
Characteristics
Variable type Dwarf nova[1]
Orbit[3]
Period (P)1.32 hours
Inclination (i)45°
Database references
SIMBADdata

Variability

The variability of LL Andromedae is similar to the WZ Sagittae type of dwarf novae. Those have a long outbursts cycle (they were observed only in 1979, 1994 and 2004)[4] and superhumps can be observed with a short periodic modulation. It was observed also a periodicity of 1.32 hours, which is attributed to the orbital period of the system. However, in comparison to WZ Sagittae, the outburst amplitude is small and the superoutbursts duration is short.[2]

System

Little is known about the components of LL Andromedae because it's a faint object; one of the two components is likely an accreting white dwarf like in all dwarf novae. A brown dwarf donor has been proposed, but the short periodicity of superhumps hints instead at the presence of a massive companion.[2]

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gollark: Maths is good, though - my maths set has a really good teacher and we do (well, did when school was running) interesting and challenging stuff a lot of the time without repeating the same topic over and over again.
gollark: English is awful because we mostly overanalyze literature and write essays and stuff, but we did writing one time and that was fun.
gollark: A lot of the chemistry and physics stuff we do at school is... somewhat interesting at first, but we end up going over it again and again and doing endless worksheets for some reason, which is not very interesting.
gollark: They might actually be actively negative in some areas, since for quite a lot of people being forced to learn the boring stuff they don't care about will make them ignore the interesting bits.

References
  1. Database entry, Catalog of Cataclysmic Variables (Downes+ 2001-2006), R. A. Downes et al., CDS ID V/123A Accessed on line 2018-11-13.
  2. Kato, T. (March 2004). "1993 Superoutburst of LL Andromedae". Publications of the Astronomical Society of Japan. 56: S135–S139. arXiv:astro-ph/0310626. Bibcode:2004PASJ...56S.135K. doi:10.1093/pasj/56.sp1.S135.
  3. Otulakowska-Hypka, M.; Olech, A.; Patterson, J. (May 1998). "Statistical analysis of properties of dwarf novae outbursts". Monthly Notices of the Royal Astronomical Society. 460 (3): 316–320. arXiv:1605.02937. Bibcode:2016MNRAS.460.2526O. doi:10.1093/mnras/stw1120.
  4. Kato, T.; et, al. (December 2009). "Survey of Period Variations of Superhumps in SU UMa-Type Dwarf Novae". Publications of the Astronomical Society of Japan. 61 (sp2): S395–S616. Bibcode:2009PASJ...61S.395K. doi:10.1093/pasj/61.sp2.S395.
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