Star in the constellation Andromeda
Phase-foldedlight curve of the RR Lyrae variable SW Andromedae recorded by NASA'sTransiting Exoplanet Survey Satellite (TESS) Light curve of SW AND taken through a J/C V band filter SW Andromedae is avariable star in the constellation ofAndromeda . It is classified as anRR Lyrae star , and varies from anapparent magnitude of 10.09 at minimum brightness to a magnitude of 9.14 at maximum brightness with a period of 0.44226 days.[ 2] Blazhko effect , and its period is decreasing.[ 6] [ 7]
The discovery of this star byAnnie Jump Cannon was announced in 1907. 461photographic plates , spanning the time interval from November 14, 1889 through November 16, 1906 were examined, and an initial period of 0.49932 days was derived.[ 8] variable star designation in 1907.[ 9]
^a b c d e f g h Since SW Andromedae is a variable star these magnitudes are means sampled over the light curve. ^a b c d e Brown, A. G. A. ; et al. (Gaia collaboration) (2021)."Gaia Early Data Release 3: Summary of the contents and survey properties" .Astronomy & Astrophysics 649 : A1.arXiv :2012.01533 Bibcode :2021A&A...649A...1G .doi :10.1051/0004-6361/202039657 S2CID 227254300 . (Erratum: doi :10.1051/0004-6361/202039657e ) . Gaia EDR3 record for this source atVizieR .^a b c SW And , database entry, Combined General Catalog of Variable Stars (GCVS4.2, 2004 Ed.), N. N. Samus, O. V. Durlevich, et al.,CDS IDII/250 Accessed on line 2014-07-02.^a b c d e f g h i Monson, Andrew J.; et al. (2017)."Standard Galactic Field RR Lyrae. I. Optical to Mid-infrared Phased Photometry" .The Astronomical Journal .153 (3). 96.arXiv :1703.01520 Bibcode :2017AJ....153...96M .doi :10.3847/1538-3881/153/3/96 S2CID 59322123 . ^a b Barcza, S.; Benkő, J. M. (2014)."Fundamental parameters of RR Lyrae stars from multicolour photometry and Kurucz atmospheric models – III. SW And, DH Peg, CU Com and DY Peg" .Monthly Notices of the Royal Astronomical Society .442 (2):1863– 1876.arXiv :1405.4184 Bibcode :2014MNRAS.442.1863B .doi :10.1093/mnras/stu978 S2CID 119182612 . ^ "V* SW And" .SIMBAD Centre de données astronomiques de Strasbourg . Retrieved2018-04-21 .^ McNamara, D. H.; Feltz, K. A., Jr. (October 1977)."A photometric study of SW Andromedae" .Publications of the Astronomical Society of the Pacific .89 :699– 703.Bibcode :1977PASP...89..699M .doi :10.1086/130212 . Retrieved5 November 2024 . {{cite journal }}: CS1 maint: multiple names: authors list (link )^ Skarka, M. (February 2014)."Bright Blazhko RRab Lyrae stars observed by ASAS and the SuperWASP surveys" (PDF) .Astronomy & Astrophysics .562 : A90.arXiv :1402.3111 Bibcode :2014A&A...562A..90S .doi :10.1051/0004-6361/201322491 . Retrieved5 November 2024 . ^ Fleming, Williamina; Cannon, Annie J.; Wells, L. D.; Pickering, Edward C. (January 1907)."Stars Having Peculiar Spectra. 18 New Variable Stars" .Harvard College Observatory Circular .124 :1– 4.Bibcode :1907HarCi.124....1F . Retrieved5 November 2024 . ^ Duné; Hartwig; Müller (November 1907)."Benennung von neu entdeckten veränderlichen Sternen" .Astronomische Nachrichten .176 (12):181– 194.Bibcode :1907AN....176..181. .doi :10.1002/asna.19071761202 . Retrieved5 November 2024 .
This variable star–related article is astub . You can help Wikipedia byexpanding it .
