Hubbry Logo
search
search button
Sign in
Historyarrow-down
starMorearrow-down
Hubbry Logo
search
search button
Sign in
DM Lyrae
Community hub for the Wikipedia article
logoWikipedian hub
Welcome to the community hub built on top of the DM Lyrae Wikipedia article. Here, you can discuss, collect, and organize anything related to DM Lyrae. The purpose of the hub is to connect people, foster deeper knowledge, and help improve the root Wikipedia article.
Add your contribution
Inside this hub
DM Lyrae
DM Lyrae

A visual band light curve for DM Lyrae, adapted from Nogami et al. (2003).[1] The inset plot shows the superhump variations.
Observation data
Epoch J2000.0      Equinox J2000.0
Constellation Lyra
Right ascension 18h 58m 44.43s[2]
Declination +30° 15′ 33.0″[2]
Apparent magnitude (V) +18 (quiet), +13.6 (burst)[2]
Characteristics
Spectral type ? / White dwarf
Variable type SU UMa[1]
Orbit[3]
Period (P)0.0654092±0.000002 d
Periastron epoch (T)2,451,343.8565±0.0015 HJD
Semi-amplitude (K1)
(primary)
37±5 km/s
Details
Donor star
Mass0.095±0.022[4] M
Radius0.145±0.011[4] R
Other designations
Lyr 1928, AN 250.1929, 1RXS J185845.1+301548, AAVSO 1854+30, DM Lyr[5]
Database references
SIMBADdata

DM Lyrae (DM Lyr for short) is a dwarf nova in the constellation Lyra. This binary system is composed of a primary star of unknown type, and a white dwarf companion. It erupted in 1928 and 1996 and reached about magnitude 13.[1]

See also

[edit]

References

[edit]
[edit]
Add your contribution
Related Hubs