S Canis Minoris

{{Short description|Variable star in the constellation Canis Minor}}{{Starbox begin}}

{{Starbox image

| image = 250px

| caption = The visual band light curve of S Canis Minoris, from AAVSO data

}}

{{Starbox observe

| constell = Canis Minor

| epoch = J2000

| ra = {{RA|07|32|43.06942}}

| dec = {{DEC|+08|19|05.1975}}

| appmag_v = 6.5 to 13.7

}}

{{Starbox character

| type = AGB

| class = M7-8e

| b-v = {{Val|1.50|0.51}}

| variable = Mira variable

}}

{{Starbox astrometry

| radial_v = {{Val|68.0|4.8}}

| prop_mo_ra = −10.785

| prop_mo_dec = −12.827

| pm_footnote =

| parallax = 2.440

| p_error = 0.098

| parallax_footnote =

| dist_footnote =

| absmag_v =

}}

{{Starbox detail

| source =

| radius = 378{{snd}}402

| luminosity = {{val|6174|402|378|fmt=commas}}

| temperature = 2,854{{snd}}2,872

| metal_fe = +0.39

| rotational_velocity =

| gravity = {{val|-0.46}} to {{Val|-0.51}}

| age_gyr =

}}

{{Starbox catalog

| names = {{odlist | BD=+08°1800 | V=S CMi | HD=59950 | HIP=36675 | SAO=115591 | AAVSO=0727+08 }}

}}

{{Starbox reference

| Simbad = S+CMi

}}

{{Starbox end}}

S Canis Minoris is a variable star in the equatorial constellation Canis Minor. It has a peak apparent visual magnitude of 6.5, so not normally visible to the naked eye. The star is located at a distance of approximately 1,340 light-years from the Sun based on stellar parallax, and is drifting further away with a radial velocity of about +68 km/s.

In 1856, John Russell Hind discovered that S Canis Minoris is a variable star. This is an aging red giant star with a stellar classification of M7-8e, where the 'e' suffix indicates emission lines in the spectrum. It is a Mira-type long period variable that varies by an amplitude of 4.27 in visual magnitude over a period of {{Val|327.77|2.78|u=days}}. Evidence has been found of asymmetry in this star, suggesting a non-spherical shape. Abundance-wise, it is an oxygen-rich giant and the emission feature is of the oxygen-rich silicate class as it sheds silicate dust from its atmosphere. The star is shedding mass at the rate of {{Val|4.9|e=−8|ul=solar mass|up=yr}}.

References

{{Reflist|refs=

{{cite Gaia DR3|3143124657116728448}}

{{cite journal |last1=Cannon |first1=Annie J. |title=Second catalogue of variable stars |journal=Annals of Harvard College Observatory |date=1907 |volume=55 |pages=1–94 |bibcode=1907AnHar..55....1C }}

{{cite web |title=Download Data |url=https://www.aavso.org/data-download |website=aavso.org |publisher=AAVSO |access-date=1 October 2021}}

{{cite simbad | title=S CMi | access-date=2019-12-13 }}

{{Cite journal |last1=Béguin |first1=E. |last2=Chiavassa |first2=A. |last3=Ahmad |first3=A. |last4=Freytag |first4=B. |last5=Uttenthaler |first5=S. |date=2024-10-01 |title=Retrieving stellar parameters and dynamics of AGB stars with Gaia parallax measurements and CO5BOLD RHD simulations |journal=Astronomy & Astrophysics |language=en |volume=690 |pages=A125 |doi=10.1051/0004-6361/202450245 |doi-access=free |arxiv=2409.03422 |issn=0004-6361}}

{{cite journal

| bibcode=2022yCat.1354....0A

| title=VizieR Online Data Catalog: StarHorse2, Gaia EDR3 photo-astrometric distances (Anders+, 2022)

| last1=Anders |first1=F. |last2=Khalatyan |first2=A.

| last3=Queiroz |first3=A. B. A. |last4=Chiappini |first4=C.

| last5=Ardevol |first5=J. |last6=Casamiquela |first6=L.

| last7=Figueras |first7=F. |last8=Jimenez-Arranz |first8=O.

| last9=Jordi |first9=C. |last10=Monguio |first10=M.

| last11=Romero-Gomez |first11=M. |last12=Altamirano |first12=D.

| last13=Antoja |first13=T. |last14=Assaad |first14=R.

| last15=Cantat-Gaudin |first15=T. |last16=Castro-Ginard |first16=A.

| last17=Enke |first17=H. |last18=Girardi |first18=L.

| last19=Guiglion |first19=G. |last20=Khan |first20=S.

| last21=Luri |first21=X. |last22=Miglio |first22=A.

| last23=Minchev |first23=I. |last24=Ramos |first24=P.

| last25=Santiago |first25=B. X. |last26=Steinmetz |first26=M.

| journal=Vizier Online Data Catalog |year=2022 }}

{{cite XHIP|32349}}

{{cite book

| first=Robert A. | last=Garfinkle

| title=Star-hopping: your Visa to Viewing the Universe

| publisher=Cambridge University Press

|location=Cambridge, United Kingdom

| year=1997 | pages=78–81

| isbn = 978-0-521-59889-7 }}

{{cite journal

| display-authors=1 | last1=Keenan | first1=Philip C.

| last2=Garrison | first2=Robert F. | last3=Deutsch | first3=Armin J.

| title=Revised Catalog of Spectra of Mira Variables of Types ME and Se

| journal=The Astrophysical Journal Supplement Series

| volume=28 | pages=271 | year=1974

| bibcode=1974ApJS...28..271K | doi=10.1086/190318 | doi-access=free }}

{{cite journal

| title=Determination of Pulsation Periods and Other Parameters of 2875 Stars Classified as MIRA in the All Sky Automated Survey (ASAS)

| last1=Vogt | first1=N. | last2=Contreras-Quijada | first2=A.

| last3=Fuentes-Morales | first3=I. | last4=Vogt-Geisse | first4=S.

| last5=Arcos | first5=C. | last6=Abarca | first6=C.

| last7=Agurto-Gangas | first7=C. | last8=Caviedes | first8=M.

| last9=DaSilva | first9=H. | last10=Flores | first10=J.

| last11=Gotta | first11=V. | last12=Peñaloza | first12=F.

| last13=Rojas | first13=K. | last14=Villaseñor | first14=J. I.

| journal=The Astrophysical Journal Supplement Series

| volume=227 | issue=1 | id=6 | pages=13 | date=November 2016

| doi=10.3847/0067-0049/227/1/6 | arxiv=1609.05246

| bibcode=2016ApJS..227....6V | s2cid=119295645 | doi-access=free }}

{{cite journal

| last1=Gontcharov | first1=G. A.

| title=Pulkovo Compilation of Radial Velocities for 35495 Hipparcos stars in a common system

| journal=Astronomy Letters

| volume=32| issue=11| pages=759–771| date=November 2006

| bibcode=2006AstL...32..759G | arxiv=1606.08053

| doi = 10.1134/S1063773706110065 | s2cid=119231169

}}

{{cite journal

| display-authors=1 | last1=Samus | first1=N. N.

| last2=Kazarovets | first2=E. V. | last3=Durlevich | first3=O. V.

| last4=Kireeva | first4=N. N. | last5=Pastukhova | first5=E. N.

| title=General Catalogue of Variable Stars

| version=5.1 | journal=Astronomy Reports

| year=2017 | volume=61 | issue=1 | pages=80–88

| bibcode=2017ARep...61...80S | doi=10.1134/S1063772917010085 | s2cid=125853869 }}

{{cite journal

| title=Mass-loss from dusty, low outflow-velocity AGB stars. I. Wind structure and mass-loss rates

| display-authors=1 | last1=Winters | first1=J. M.

| last2=Le Bertre | first2=T. | last3=Jeong | first3=K. S.

| last4=Nyman | first4=L. -Å. | last5=Epchtein | first5=N.

| journal=Astronomy and Astrophysics

| volume=409 | pages=715–735 | date=October 2003

| issue=2 | doi=10.1051/0004-6361:20031110 | bibcode=2003A&A...409..715W | doi-access=free }}

{{cite journal

| title=The Infrared Spectral Classification of Oxygen-rich Dust Shells

| last1=Sloan | first1=G. C. | last2=Price | first2=S. D.

| journal=The Astrophysical Journal Supplement Series

| volume=119 | issue=2 | pages=141–158 | date=December 1998

| doi=10.1086/313156 | bibcode=1998ApJS..119..141S | doi-access=free }}

{{cite journal

| title=New observations and models of circumstellar CO line emission of AGB stars in the Herschel SUCCESS programme

| display-authors=1 | last1=Danilovich | first1=T.

| last2=Teyssier | first2=D. | last3=Justtanont | first3=K.

| last4=Olofsson | first4=H. | last5=Cerrigone | first5=L.

| last6=Bujarrabal | first6=V. | last7=Alcolea | first7=J.

| last8=Cernicharo | first8=J. | last9=Castro-Carrizo | first9=A.

| last10=García-Lario | first10=P. | last11=Marston | first11=A.

| journal=Astronomy & Astrophysics

| volume=581 | id=A60 | pages=33 | date=September 2015

| doi=10.1051/0004-6361/201526705 | arxiv=1506.09065

| bibcode=2015A&A...581A..60D | s2cid=55109956 }}

}}

{{Stars of Canis Minor}}

{{DEFAULTSORT:S Canis Minoris}}

Category:M-type giants

Category:Mira variables

Category:Canis Minor

Category:Durchmusterung objects

059950

036675

Canis Minoris, S

Category:Emission-line stars