From Wikipedia, the free encyclopedia
Variable star in the constellation Reticulum
R Reticuli , also listed under the duplicate
variable star designation S Reticuli ,
[4] is a
Mira variable star in the southern
constellation
Reticulum . It is an aging
red giant star on the
asymptotic giant branch
[5] with a
stellar classification that varies between M4e to M7.5e,
[6] being hottest near maximum visual magnitude.
[10] The brightness of the star varies between
apparent visual magnitudes 6.35 and 14.2
[4] with an average period of 281.08± 0.58 d .
[11] The mean maximum magnitude is 7.57 and the mean minimum magnitude 13.80.
[11]
References
^
"Download Data" . aavso.org . AAVSO. Retrieved 1 October 2021 .
^
a
b
c
d
e Vallenari, A.; et al. (Gaia collaboration) (2023).
"Gaia Data Release 3. Summary of the content and survey properties" . Astronomy and Astrophysics . 674 : A1.
arXiv :
2208.00211 .
Bibcode :
2023A&A...674A...1G .
doi :
10.1051/0004-6361/202243940 .
S2CID
244398875 .
Gaia DR3 record for this source at
VizieR .
^
a
b
c Anderson, E.; Francis, Ch. (2012). "XHIP: An extended hipparcos compilation". Astronomy Letters . 38 (5): 331.
arXiv :
1108.4971 .
Bibcode :
2012AstL...38..331A .
doi :
10.1134/S1063773712050015 .
S2CID
119257644 .
^
a
b
c VSX; Otero, S. A. (28 January 2011).
"R Reticuli" . AAVSO Website .
American Association of Variable Star Observers . Retrieved 25 May 2014 .
^
a
b Whitelock, Patricia A.; et al. (May 2008). "AGB variables and the Mira period-luminosity relation". Monthly Notices of the Royal Astronomical Society . 386 (1): 313–323.
arXiv :
0801.4465 .
Bibcode :
2008MNRAS.386..313W .
doi :
10.1111/j.1365-2966.2008.13032.x .
S2CID
17676993 .
^
a
b
c Samus, N. N.; et al. (2017). "General Catalogue of Variable Stars". Astronomy Reports . 5.1. 61 (1): 80–88.
Bibcode :
2017ARep...61...80S .
doi :
10.1134/S1063772917010085 .
S2CID
125853869 .
^
a
b
c Anders, F.; Khalatyan, A.; Chiappini, C.; Queiroz, A. B.; Santiago, B. X.; Jordi, C.; Girardi, L.; Brown, A. G. A.; Matijevič, G.; Monari, G.; Cantat-Gaudin, T.; Weiler, M.; Khan, S.; Miglio, A.; Carrillo, I.; Romero-Gómez, M.; Minchev, I.; De Jong, R. S.; Antoja, T.; Ramos, P.; Steinmetz, M.; Enke, H. (2019). "Photo-astrometric distances, extinctions, and astrophysical parameters for Gaia DR2 stars brighter than G = 18". Astronomy and Astrophysics . 628 : A94.
arXiv :
1904.11302 .
Bibcode :
2019A&A...628A..94A .
doi :
10.1051/0004-6361/201935765 .
S2CID
131780028 .
^
a
b
c
Brown, A. G. A. ; et al. (Gaia collaboration) (August 2018).
"Gaia Data Release 2: Summary of the contents and survey properties" .
Astronomy & Astrophysics . 616 . A1.
arXiv :
1804.09365 .
Bibcode :
2018A&A...616A...1G .
doi :
10.1051/0004-6361/201833051 .
Gaia DR2 record for this source at
VizieR .
^
"R Ret" .
SIMBAD .
Centre de données astronomiques de Strasbourg . Retrieved 2020-11-18 .
^ Skiff, B. A. (2014). "VizieR Online Data Catalog: Catalogue of Stellar Spectral Classifications (Skiff, 2009- )". VizieR On-line Data Catalog .
Bibcode :
2014yCat....1.2023S .
^
a
b Vogt, N.; et al. (November 2016).
"Determination of Pulsation Periods and Other Parameters of 2875 Stars Classified as MIRA in the All Sky Automated Survey (ASAS)" . The Astrophysical Journal Supplement Series . 227 (1): 13.
arXiv :
1609.05246 .
Bibcode :
2016ApJS..227....6V .
doi :
10.3847/0067-0049/227/1/6 .
S2CID
119295645 . 6.