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{{Short description|Star in the constellation Antlia}}
{{Starbox short |
{{Starbox begin
| name=UX Antliae
| name=UX Antliae
| epoch=[[J2000.0]]
| constell=[[Antlia]]
| ra=10<sup>h</sup> 57<sup>m</sup> 09.06<sup>s</sup>
| dec= -37° 23' 55.0"
| spectral= hglsg
| appmag_v=12.6
| dist_ly=700 ± 86
| dist_pc=
| names=[[Guide Star Catalog II|GSC2]] S1303203939, [[2MASS]] J10570905-3723550, [[Tycho Catalogue|TYC]] 7212-77-1, [[DENIS-P]] J105709.0-372354, [[Guide Star Catalog|GSC]] 07212-00077, [[HV (star catalog)|HV]] 10108, [[AAVSO]] 1052-36
| Simbad =UX+Antliae
| ARICNS =
}}
}}
{{Starbox image
| image = [[Image:UXAntLightCurve.png|250px]]
| caption = The [[Photometric_system#Photometric_letters|visual band]] [[light curve]] of UX Antliae, from AAVSO data<ref name=download/>
}}
{{Starbox observe
| epoch=J2000.0
| ra={{RA|10|57|9.051}}<ref name=tycho2/>
| dec={{DEC|-37|23|55.06}}<ref name=tycho2/>
| appmag_v=11.85 - 18.0<ref name=aavso/>
| constell=[[Corona Borealis]]
}}
{{Starbox character
| class=C(F)<ref name=lawson/>
| b-v=
| u-b=
| v-r=
| j-h=
| j-k=
| variable=[[R Coronae Borealis variable|R CrB]]<ref name=hema/>}}
{{Starbox astrometry
| radial_v=27.83<ref name=white/>
| prop_mo_ra=-3.8<ref name=tycho2/>
| prop_mo_dec=2.3<ref name=tycho2/>
| parallax=
| p_error=
| parallax_footnote=
| dist_pc=~25,000<ref name=lawson/>
| dist_ly=
| absmag_v=~&minus;5<ref name=lawson/>
}}
{{Starbox detail
| mass=0.722<ref name=stasinska/>
| radius=
| luminosity=
| temperature=7,000<ref name=stasinska/>
| metal=
| gravity=0.5<ref name=stasinska/>
| rotation=
| age=
}}
{{Starbox catalog
| names=[[2MASS]]&nbsp;J10570905-3723550, [[Tycho Catalogue|TYC]]&nbsp;7212-77-1, [[HV (star catalog)|HV]]&nbsp;10108, [[DENIS-P]]&nbsp;J105709.0-372354, [[Guide Star Catalog|GSC]]&nbsp;07212-00077, [[Guide Star Catalog II|GSC2]]&nbsp;S1303203939, [[AAVSO]]&nbsp;1052-36
}}
{{Starbox reference
| Simbad=UX+Ant
}}
{{Starbox end}}



'''UX Antliae''' is [[Protoplanetary nebula|post-AGB star]]. Variable star [[R Coronae Borealis]] type.
'''UX Antliae''' is a [[Protoplanetary nebula|post-AGB]] and [[R Coronae Borealis variable]] star that has a base [[apparent magnitude]] of around 11.85, with irregular dimmings down to below magnitude 18.0.<ref name=aavso2/>

Researchers David Kilkenny and J.E. Westerhuys of the [[South African Astronomical Observatory]] confirmed that UX Antliae was an R Coronae Borealis variable in 1990 after noting the similarity of its spectrum to the RCB star [[W Mensae]].<ref name=Kilkenny90/> It had been suspected of being one since 1940, but had been little-studied and exhibited no characteristic declines between 1975 and 1990.<ref name=lawson/>

Assuming that its absolute magnitude is around -5, it has been estimated as lying 25000 parsecs distant from Earth.<ref name=lawson/> Kilkenny and Westerhuys noted that its spectrum fit with that of a star of spectral class F, although was deficient in hydrogen.<ref name=Kilkenny90/> It has around 70% the mass of the Sun and an [[effective temperature|effective (surface) temperature]] of around 7000 K.<ref name="stasinska"/>

==See also==
*[[R Coronae Borealis]]


==References==
==References==
{{reflist|refs=


<ref name="stasinska">{{cite journal|bibcode=2006A&A...450..701S|title=Post-AGB stars as testbeds of nucleosynthesis in AGB stars|journal=Astronomy and Astrophysics|volume=450|issue=2|pages=701|last1=Stasińska|first1=G.|last2=Szczerba|first2=R.|last3=Schmidt|first3=M.|last4=Siódmiak|first4=N.|date=2006|doi=10.1051/0004-6361:20053553|arxiv = astro-ph/0601504 |s2cid=12040452}}</ref>
* {{cite journal|author=Lawson, W. A., Cottrell, P. L., Kilkenny, D., Gilmore, A. C., Kilmartin, P. M.|title=The Variability of the R-Coronae Star Ux-Antliae at Maximum Light|journal=Mon. Not. R. Astron. Soc.|volume=271|pages=919&ndash;923|year=1994|bibcode=1994MNRAS.271..919L|last2=Cottrell|last3=Kilkenny|last4=Gilmore|last5=Kilmartin|last6=Marang|last7=Roberts|last8=Van Wyk }}


<ref name=lawson>{{cite journal|author=Lawson, W. A.|author2=Cottrell, P. L.|author3=Kilkenny, D.|author4=Gilmore, A. C.|author5=Kilmartin, P. M.|title=The Variability of the R-Coronae Star Ux-Antliae at Maximum Light|journal=Mon. Not. R. Astron. Soc.|volume=271|issue=4|pages=919–23|date=1994|bibcode=1994MNRAS.271..919L|last6=Marang|last7=Roberts|last8=Van Wyk|doi=10.1093/mnras/271.4.919|doi-access=free}}</ref>
* {{cite web | url=http://aladin.u-strasbg.fr/AladinPreview?-c=10+57+09.06-37+23+55.0&ident=V*+UX+Ant&submit=Aladin+previewer | title=Image UX Antliae | work=[[SIMBAD]] | accessdate=}}
* {{cite web | url=http://www.ncac.torun.pl/postagb?lang=en&branch=postagbworld&id=2&l=279.064&b=20.12 | title=Post-AGB Object 279.064 +20.120 | work=www.ncac.torun.pl | accessdate=}}


<ref name=Kilkenny90>{{cite journal|author=Kilkenny, D.|author2=Westerhuys, J. E. |date=1990|title= Spectroscopy of 'RCB' stars-IV. UX ANT |journal= The Observatory|volume=110 |pages=90–92|bibcode = 1990Obs...110...90K }}</ref>
* {{cite web | url=http://www.kusastro.kyoto-u.ac.jp/vsnet/LCs/index/ANTUX.html | title=Light Curve of UX Ant | work=www.kusastro.kyoto-u.ac.jp | accessdate=}}


<ref name=aavso2>{{ cite web | title= V4199 Sgr | work=The International Variable Star Index | url=http://www.aavso.org/vsx/index.php?view=detail.top&oid=31899| author=Otero, Sebastian | date=23 November 2012 | access-date=14 July 2014}}</ref>
* {{cite web | url=http://vsnet.kusastro.kyoto-u.ac.jp/vsnet/Mail/vsnet-rcb/msg00584.html | title=message | work=vsnet.kusastro.kyoto-u.ac.jp | accessdate=}}


<ref name=stasinska>{{cite journal|bibcode=2006A&A...450..701S|title=Post-AGB stars as testbeds of nucleosynthesis in AGB stars|journal=Astronomy and Astrophysics|volume=450|issue=2|pages=701|last1=Stasińska|first1=G.|last2=Szczerba|first2=R.|last3=Schmidt|first3=M.|last4=Siódmiak|first4=N.|date=2006|doi=10.1051/0004-6361:20053553|arxiv = astro-ph/0601504 |s2cid=12040452}}</ref>
[[Category:Antlia (constellation)]]
[[Category:R Coronae Borealis variables]]
[[Category:Objects named with variable star designations|Antliae, UX]]


<ref name=white>{{cite journal|bibcode=2007AJ....133.2524W|title=High-Dispersion Optical Spectra of Nearby Stars Younger Than the Sun|journal=The Astronomical Journal|volume=133|issue=6|pages=2524|last1=White|first1=Russel J.|last2=Gabor|first2=Jared M.|last3=Hillenbrand|first3=Lynne A.|date=2007|doi=10.1086/514336|arxiv = 0706.0542 |s2cid=122854}}</ref>
{{var-star-stub}}

<ref name=aavso>{{ cite web | title= UX Antliae | work=The International Variable Star Index | url=http://www.aavso.org/vsx/index.php?view=detail.top&oid=31899| author=Otero, Sebastian | date=23 November 2012 | access-date=14 July 2014}}</ref>

<ref name=tycho2>{{cite journal|bibcode=2000A&A...355L..27H|title=The Tycho-2 catalogue of the 2.5 million brightest stars|journal=Astronomy and Astrophysics|volume=355|pages=L27|last1=Høg|first1=E.|last2=Fabricius|first2=C.|last3=Makarov|first3=V. V.|last4=Urban|first4=S.|last5=Corbin|first5=T.|last6=Wycoff|first6=G.|last7=Bastian|first7=U.|last8=Schwekendiek|first8=P.|last9=Wicenec|first9=A.|date=2000|doi=10.1888/0333750888/2862}}</ref>

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

<ref name=hema>{{cite journal|bibcode=2012ApJ...747..102H|title=The Galactic R Coronae Borealis Stars: The C2 Swan Bands, the Carbon Problem, and the 12C/13C Ratio|journal=The Astrophysical Journal|volume=747|issue=2|pages=102|last1=Hema|first1=B. P.|last2=Pandey|first2=Gajendra|last3=Lambert|first3=David L.|date=2012|doi=10.1088/0004-637X/747/2/102|arxiv = 1201.1357 |s2cid=118653032}}</ref>
}}

==External links==
{{cite web | url=http://www.ncac.torun.pl/postagb?lang=en&branch=postagbworld&id=2&l=279.064&b=20.12 | title=Post-AGB Object 279.064 +20.120 | work=www.ncac.torun.pl }}<br>
{{cite web | url=http://www.kusastro.kyoto-u.ac.jp/vsnet/LCs/index/ANTUX.html | title=Light Curve of UX Ant | work=www.kusastro.kyoto-u.ac.jp }}

{{Stars of Antlia}}

{{DEFAULTSORT:UX Antliae}}
[[Category:Antlia]]
[[Category:R Coronae Borealis variables]]
[[Category:Objects with variable star designations|Antliae, UX]]
[[Category:2MASS objects|J10570905-3723550]]

Latest revision as of 00:54, 6 October 2022

UX Antliae

The visual band light curve of UX Antliae, from AAVSO data[1]
Observation data
Epoch J2000.0      Equinox J2000.0
Constellation Corona Borealis
Right ascension 10h 57m 9.051s[2]
Declination −37° 23′ 55.06″[2]
Apparent magnitude (V) 11.85 - 18.0[3]
Characteristics
Spectral type C(F)[4]
Variable type R CrB[5]
Astrometry
Radial velocity (Rv)27.83[6] km/s
Proper motion (μ) RA: -3.8[2] mas/yr
Dec.: 2.3[2] mas/yr
Distance~25,000[4] pc
Absolute magnitude (MV)~−5[4]
Details
Mass0.722[7] M
Surface gravity (log g)0.5[7] cgs
Temperature7,000[7] K
Other designations
2MASS J10570905-3723550, TYC 7212-77-1, HV 10108, DENIS-P J105709.0-372354, GSC 07212-00077, GSC2 S1303203939, AAVSO 1052-36
Database references
SIMBADdata


UX Antliae is a post-AGB and R Coronae Borealis variable star that has a base apparent magnitude of around 11.85, with irregular dimmings down to below magnitude 18.0.[8]

Researchers David Kilkenny and J.E. Westerhuys of the South African Astronomical Observatory confirmed that UX Antliae was an R Coronae Borealis variable in 1990 after noting the similarity of its spectrum to the RCB star W Mensae.[9] It had been suspected of being one since 1940, but had been little-studied and exhibited no characteristic declines between 1975 and 1990.[4]

Assuming that its absolute magnitude is around -5, it has been estimated as lying 25000 parsecs distant from Earth.[4] Kilkenny and Westerhuys noted that its spectrum fit with that of a star of spectral class F, although was deficient in hydrogen.[9] It has around 70% the mass of the Sun and an effective (surface) temperature of around 7000 K.[7]

See also

[edit]

References

[edit]
  1. ^ "Download Data". aavso.org. AAVSO. Retrieved 1 October 2021.
  2. ^ a b c d Høg, E.; Fabricius, C.; Makarov, V. V.; Urban, S.; Corbin, T.; Wycoff, G.; Bastian, U.; Schwekendiek, P.; Wicenec, A. (2000). "The Tycho-2 catalogue of the 2.5 million brightest stars". Astronomy and Astrophysics. 355: L27. Bibcode:2000A&A...355L..27H. doi:10.1888/0333750888/2862.
  3. ^ Otero, Sebastian (23 November 2012). "UX Antliae". The International Variable Star Index. Retrieved 14 July 2014.
  4. ^ a b c d e Lawson, W. A.; Cottrell, P. L.; Kilkenny, D.; Gilmore, A. C.; Kilmartin, P. M.; Marang; Roberts; Van Wyk (1994). "The Variability of the R-Coronae Star Ux-Antliae at Maximum Light". Mon. Not. R. Astron. Soc. 271 (4): 919–23. Bibcode:1994MNRAS.271..919L. doi:10.1093/mnras/271.4.919.
  5. ^ Hema, B. P.; Pandey, Gajendra; Lambert, David L. (2012). "The Galactic R Coronae Borealis Stars: The C2 Swan Bands, the Carbon Problem, and the 12C/13C Ratio". The Astrophysical Journal. 747 (2): 102. arXiv:1201.1357. Bibcode:2012ApJ...747..102H. doi:10.1088/0004-637X/747/2/102. S2CID 118653032.
  6. ^ White, Russel J.; Gabor, Jared M.; Hillenbrand, Lynne A. (2007). "High-Dispersion Optical Spectra of Nearby Stars Younger Than the Sun". The Astronomical Journal. 133 (6): 2524. arXiv:0706.0542. Bibcode:2007AJ....133.2524W. doi:10.1086/514336. S2CID 122854.
  7. ^ a b c d Stasińska, G.; Szczerba, R.; Schmidt, M.; Siódmiak, N. (2006). "Post-AGB stars as testbeds of nucleosynthesis in AGB stars". Astronomy and Astrophysics. 450 (2): 701. arXiv:astro-ph/0601504. Bibcode:2006A&A...450..701S. doi:10.1051/0004-6361:20053553. S2CID 12040452.
  8. ^ Otero, Sebastian (23 November 2012). "V4199 Sgr". The International Variable Star Index. Retrieved 14 July 2014.
  9. ^ a b Kilkenny, D.; Westerhuys, J. E. (1990). "Spectroscopy of 'RCB' stars-IV. UX ANT". The Observatory. 110: 90–92. Bibcode:1990Obs...110...90K.
[edit]

"Post-AGB Object 279.064 +20.120". www.ncac.torun.pl.
"Light Curve of UX Ant". www.kusastro.kyoto-u.ac.jp.