Delta Circini

{{Short description|Variable star in the constellation Circinus}}

{{Starbox begin

| name = Delta Circini

}}

{{Starbox image

| image=

{{Location mark

|image=Circinus constellation map.svg

|float=center

|alt=

|label=

|position=right

|width=260

|mark=Red circle.svg

|mark_width=10

|mark_link=δ Circini

|x=361|y=522

}}

|caption=Location of δ Cir (circled)

}}

{{Starbox observe

| epoch = J2000.0

| constell = Circinus

| ra = {{RA|15|16|56.89591}}

| dec = {{DEC|-60|57|26.1201}}

| appmag_v = 5.09{{cite journal|bibcode= 2002yCat.2237....0D |title= VizieR Online Data Catalog: Catalogue of Stellar Photometry in Johnson's 11-color system |journal= CDS/ADC Collection of Electronic Catalogues |volume= 2237 |last1= Ducati |first1= J. R. |year= 2002 }} {{nowrap|(5.05 - 5.20)}}

}}

{{Starbox character

| class = O7.5III(f) {{nowrap|(O8IV + O9.5V + B0.5V({{cite journal|bibcode=2001ApJ...548..889P|title=Tomographic Separation of Composite Spectra. VII. The Physical Properties of the Massive Triple System HD 135240 (δ Circini)|journal=The Astrophysical Journal|volume=548|issue=2|pages=889|last1=Penny|first1=Laura R.|last2=Seyle|first2=Debra|last3=Gies|first3=Douglas R.|last4=Harvin|first4=James A.|last5=Bagnuolo|first5=William G.|last6=Thaller|first6=M. L.|last7=Fullerton|first7=A. W.|last8=Kaper|first8=L.|year=2001|doi=10.1086/319031|doi-access=free}})}}

| b-v = −0.06

| u-b = −0.88

| variable = Eclipsing and ellipsoidal

}}

{{Starbox astrometry

| radial_v = −17.80{{cite journal|bibcode=2004A&A...424..727P|title=SB9: The ninth catalogue of spectroscopic binary orbits|journal=Astronomy and Astrophysics|volume=424|issue=2|pages=727–732|last1=Pourbaix|first1=D.|last2=Tokovinin|first2=A. A.|last3=Batten|first3=A. H.|last4=Fekel|first4=F. C.|last5=Hartkopf|first5=W. I.|last6=Levato|first6=H.|last7=Morrell|first7=N. I.|last8=Torres|first8=G.|last9=Udry|first9=S.|year=2004|doi=10.1051/0004-6361:20041213|arxiv = astro-ph/0406573 |s2cid=119387088}}

| prop_mo_ra = −4.085

| prop_mo_dec = −3.758

| parallax = 1.4345

| p_error = 0.1231

| parallax_footnote={{cite Gaia DR3|5875491419647525248}}

| dist_pc =

| absmag_v =

}}

{{Starbox orbit

| reference =

| primary = Aa

| name = Ab

| period =

| period_unitless = 3.902463 days

| axis =

| axis_unitless = {{solar radius|34.7}}

| eccentricity = 0.068

| inclination = 75.81

| node =

| periastron =

| periarg =

| periarg_primary =

| k1 = 156.8

| k2 = 280.4

}}

{{Starbox orbit|no_heading=y

| reference =

| primary = Aab

| name = Ac

| period =

| period_unitless = 1,644 days

| axis = 3.87

| axis_unitless =

| eccentricity = 0.415

| inclination = 87.7

| node =

| periastron =

| periarg =

| periarg_primary =

| k1 = 23.6

| k2 =

}}

{{Starbox detail

| component1=Aa

| mass={{val|20.00|0.50}}{{cite journal |title=High-mass pulsators in eclipsing binaries observed using TESS |author1=Southworth, John |author2=Bowman, Dominic M. |journal=Monthly Notices of the Royal Astronomical Society |volume=513 |issue=3 |pages=3191–3209 |date=July 2022 |bibcode=2022MNRAS.513.3191S |doi=10.1093/mnras/stac875 |doi-access=free |arxiv=2203.15365 }}

| radius={{val|9.256|0.091}}

| luminosity={{val|fmt=commas|153,000|27,000|23,000}}

| temperature=37,500

| metal=

| gravity=3.806

| rotational_velocity={{val|150|9}}

| age_myr=

}}

{{Starbox detail|no_heading=y

| component1=Ab

| mass={{val|11.41|0.24}}

| radius={{val|5.326|0.091}}

| luminosity={{val|fmt=commas|21,827|5,026|4,085}}

| temperature={{val|fmt=commas|30,400|400}}

| metal=

| gravity={{val|4.043|0.014}}

| rotational_velocity={{val|141|230}}

| age_myr=

}}

{{Starbox detail|no_heading=y

| component1=Ac

| mass=18.7

| radius=

| luminosity=17,000

| temperature=28,000

| metal=

| gravity=4.2

| rotation=

| age_myr=

}}

{{Starbox catalog

| names = δ Cir, CD−60°5539, SAO 253084, HD 135240, HR 5664, HIP 74778, WDS J15169-6057

}}

{{Starbox reference

|Simbad=del+Cir

}}

{{Starbox end}}

Delta Circini (δ Cir), is a multiple star system located in the constellation Circinus. Delta Circini is also known as HR 5664, and HD 135240. The system has a combined apparent visual magnitude of +5.09, and is located at a distance of about 700 pc (2,300ly) from the Sun.

Companions

δ Circini A is a spectroscopic triple star, although the outer component has been resolved using the VLTI PIONIER instrument. The two inner components form an eclipsing binary system.{{cite journal|bibcode=2014AJ....148..114M|title=The Three-body System δ Circini|journal=The Astronomical Journal|volume=148|issue=6|pages=114|last1=Mayer|first1=Pavel|last2=Harmanec|first2=Petr|last3=Sana|first3=Hugues|last4=Le Bouquin|first4=Jean-Baptiste|year=2014|doi=10.1088/0004-6256/148/6/114|arxiv = 1408.1958 |s2cid=118333313}}

δ Circini B is a 13th magnitude companion nearly an arc-second away. It is unclear whether the two are physically associated and little is known about the fainter star although it has been reported to be a G5 main sequence star or giant.{{cite journal|bibcode=1985A&AS...60..183L |title=A study of visual double stars with early type primaries. IV Astrophysical data |journal=Astronomy and Astrophysics Supplement Series |volume=60 |pages=183 |last1=Lindroos |first1=K. P. |year=1985 }}

HD 135160 is a 6th magnitude binary Be star that shares a common space motion with δ Circini and is only 4 arc minutes away. The two make a faint naked eye pair.

System properties

File:DeltaCirLightCurve.png for Delta Circini, plotted from TESS data{{cite web |title=MAST: Barbara A. Mikulski Archive for Space Telescopes |url=https://mast.stsci.edu/portal/Mashup/Clients/Mast/Portal.html |publisher=Space Telescope Science Institute |access-date=8 December 2021}}]]

All three components of δ Circini A are hot luminous stars. The brightest is an O8 star just beginning to evolve away from the main sequence. It is in a very close orbit with an O9.5 main sequence star. The two stars are deformed into ellipsoidal shapes and eclipse each other every 3.9 days. The total brightness change is only 0.15 magnitudes.

The third component is a B0.5 main sequence star in a long eccentric orbit around the close pair. It is fainter and cooler than either of the two close stars, yet it is calculated to be more massive than δ Cir A, so it is suspected that it may also be a close binary system.

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References

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