On the Period of the Mira Variable LX Cygni
The period changes of the SC-type Mira variable LX Cygni are analyzed.
Main Authors: | Barzdis A., Alksnis A. |
---|---|
Format: | Article |
Language: | English |
Published: |
De Gruyter
2003-12-01
|
Series: | Open Astronomy |
Subjects: | |
Online Access: | https://doi.org/10.1515/astro-2017-0092 |
Similar Items
-
Early Photometric and Spectral Evolution of Nova Cygni 2014 (V2659 Cyg)
by: Burlak M. A., et al.
Published: (2015-12-01) -
Recurrent Symbiotic Nova V407 Cygni: Before and after Outburst in 2010
by: Esipov V. F., et al.
Published: (2015-12-01) -
Variability Survey of Massive Stars in OB-Associations: Preliminary Results on the Cygnus Region
by: Laur J., et al.
Published: (2012-12-01) -
Spectroscopic Observations of the Recurrent Symbiotic Nova V407 Cyg During 2001 - 2009
by: Esipov V. F., et al.
Published: (2012-06-01) -
Half a Century after the Outburst of the Symbiotic Nova V1016 Cyg
by: Arkhipova V. P., et al.
Published: (2016-03-01)