Jump to content

4U 1543-475: Difference between revisions

From Wikipedia, the free encyclopedia
Browse history interactively
← Previous editNext edit →
Content deleted Content added
VisualWikitext
I move the references to reflist to avoid clutter.
m Here's an incomplete infobox with Gaia DR3 astrometry.
Line 1: Line 1:
{{Starbox begin
| name = [[Variable star designation|IL Lupi]]
⚫
}}
{{Starbox observe
| epoch = [[J2000.0]] ([[International Celestial Reference System|ICRS]])
| constell = [[Lupus]]
| ra = {{RA|15|47|08.27687}}<ref name = GaiaDR3/>
| dec = {{DEC|−47|40|10.2846}}<ref name = GaiaDR3/>
| appmag_v = 11.96<ref name = "Alfonso-Garzón2012"/> (14.6 - 16.7)<ref name = Samus2017/>
}}
{{Starbox character
| class =
| variable = [[X-ray binary|XNG]]<ref name = Samus2017/>
}}
{{Starbox astrometry
| radial_v =
| parallax = 0.1909
| p_error = 0.0551
| parallax_footnote = <ref name = GaiaDR3/>
| prop_mo_ra = −7.543
| prop_mo_dec = −5.356
| pm_footnote = <ref name = GaiaDR3/>
}}
{{Starbox end}}

'''4U 1543-475''' is a recurrent [[X-ray transient]].<ref name='Palombara'/> It is a member of a [[black hole]] binary and is in the [[Lupus (constellation)|constellation of Lupus]].<ref name = Kiamoto1984/> Its optical counterpart is IL Lupi.<ref name='Palombara'/> Outburst from 4U 1543-475 was first observed by [[Uhuru (satellite)|Uhuru]] in 1971.<ref name = Maltilsky1972/>
'''4U 1543-475''' is a recurrent [[X-ray transient]].<ref name='Palombara'/> It is a member of a [[black hole]] binary and is in the [[Lupus (constellation)|constellation of Lupus]].<ref name = Kiamoto1984/> Its optical counterpart is IL Lupi.<ref name='Palombara'/> Outburst from 4U 1543-475 was first observed by [[Uhuru (satellite)|Uhuru]] in 1971.<ref name = Maltilsky1972/>


Line 7: Line 32:
== References ==
== References ==
{{Reflist||refs=
{{Reflist||refs=

<ref name = GaiaDR3>{{Cite DR3|5986117923045619072}}</ref>


<ref name='Palombara'>{{cite journal |last1=Palombara |first1=Nicola La |last2=Mereghetti |first2=Sandro |date=2 February 2008 |title= XMM-Newton observation of 4U 1543–475: The X-ray spectrum of a stellar-mass black-hole at low luminosity |journal=[[Astronomy & Astrophysics]] |volume=430 |issue=2005 |pages=L53–L56 |doi=10.1051/0004-6361:200400123 |arxiv=astro-ph/0412209|bibcode=2005A&A...430L..53L |citeseerx=10.1.1.316.7094 |s2cid=865125 }}</ref>
<ref name='Palombara'>{{cite journal |last1=Palombara |first1=Nicola La |last2=Mereghetti |first2=Sandro |date=2 February 2008 |title= XMM-Newton observation of 4U 1543–475: The X-ray spectrum of a stellar-mass black-hole at low luminosity |journal=[[Astronomy & Astrophysics]] |volume=430 |issue=2005 |pages=L53–L56 |doi=10.1051/0004-6361:200400123 |arxiv=astro-ph/0412209|bibcode=2005A&A...430L..53L |citeseerx=10.1.1.316.7094 |s2cid=865125 }}</ref>
Line 15: Line 42:
|first5=H. D. |date=15 May 1972 |title=A New Transient Source Observed by UHURU |journal=[[The Astrophysical Journal]] |volume=174 |pages=L53–L55 |doi=10.1086/180947 |bibcode=1972ApJ...174L..53M}}</ref>
|first5=H. D. |date=15 May 1972 |title=A New Transient Source Observed by UHURU |journal=[[The Astrophysical Journal]] |volume=174 |pages=L53–L55 |doi=10.1086/180947 |bibcode=1972ApJ...174L..53M}}</ref>


<ref name = Samus2017>{{cite journal | 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 GCVS 5.1 | journal = Astronomy Reports | date = January 2017 | volume = 61 | issue = 1 | pages = 80–88 | issn = 1063-7729 | eissn = 1562-6881 | doi = 10.1134/S1063772917010085 | bibcode = 2017ARep...61...80S| s2cid = 125853869 }}</ref>
⚫
}}


<ref name = "Alfonso-Garzón2012">{{cite journal | last1 = Alfonso-Garzón | first1 = J. | last2 = Domingo | first2 = A. | last3 = Mas-Hesse | first3 = J. M. | last4 = Giménez | first4 = A. | title = The first INTEGRAL-OMC catalogue of optically variable sources | journal = Astronomy & Astrophysics | date = 26 November 2012 | volume = 548 | page = A79 | issn = 0004-6361 | eissn = 1432-0746 | doi = 10.1051/0004-6361/201220095 | arxiv = 1210.0821 | bibcode = 2012A&A...548A..79A | s2cid = 118428054 | doi-access = free}}</ref>

}}
{{Stars of Lupus}}
{{Stars of Lupus}}


Revision as of 16:08, 13 April 2023

IL Lupi
Observation data
Epoch J2000.0      Equinox J2000.0 (ICRS)
Constellation Lupus
Right ascension 15h 47m 08.27687s[1]
Declination −47° 40′ 10.2846″[1]
Apparent magnitude (V) 11.96[2] (14.6 - 16.7)[3]
Characteristics
Variable type XNG[3]
Astrometry
Proper motion (μ) RA: −7.543 mas/yr[1]
Dec.: −5.356 mas/yr[1]
Parallax (π)0.1909 ± 0.0551 mas[1]
Distanceapprox. 17,000 ly
(approx. 5,000 pc)

4U 1543-475 is a recurrent X-ray transient.[4] It is a member of a black hole binary and is in the constellation of Lupus.[5] Its optical counterpart is IL Lupi.[4] Outburst from 4U 1543-475 was first observed by Uhuru in 1971.[6]

See also

References

  1. ^ a b c d 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.
  2. ^ Alfonso-Garzón, J.; Domingo, A.; Mas-Hesse, J. M.; Giménez, A. (26 November 2012). "The first INTEGRAL-OMC catalogue of optically variable sources". Astronomy & Astrophysics. 548: A79. arXiv:1210.0821. Bibcode:2012A&A...548A..79A. doi:10.1051/0004-6361/201220095. eISSN 1432-0746. ISSN 0004-6361. S2CID 118428054.
  3. ^ a b Samus’, N. N.; Kazarovets, E. V.; Durlevich, O. V.; Kireeva, N. N.; Pastukhova, E. N. (January 2017). "General catalogue of variable stars: Version GCVS 5.1". Astronomy Reports. 61 (1): 80–88. Bibcode:2017ARep...61...80S. doi:10.1134/S1063772917010085. eISSN 1562-6881. ISSN 1063-7729. S2CID 125853869.
  4. ^ a b Palombara, Nicola La; Mereghetti, Sandro (2 February 2008). "XMM-Newton observation of 4U 1543–475: The X-ray spectrum of a stellar-mass black-hole at low luminosity". Astronomy & Astrophysics. 430 (2005): L53–L56. arXiv:astro-ph/0412209. Bibcode:2005A&A...430L..53L. CiteSeerX 10.1.1.316.7094. doi:10.1051/0004-6361:200400123. S2CID 865125.
  5. ^ Kitamoto, S.; Miyamoto, S.; Tsunemi, H; Makishima, K; Nakagawa, M (1 June 1984). "The transient X-ray source 4U 1543-47 observed from TENMA". Publications of the Astronomical Society of Japan. 36 (4): 799–806. Bibcode:1984PASJ...36..799K.
  6. ^ MATiLSKY, T. A.; Giacconi, R.; Gursky, H.; Kellogg, E. M.; Tananbaum, H. D. (15 May 1972). "A New Transient Source Observed by UHURU". The Astrophysical Journal. 174: L53–L55. Bibcode:1972ApJ...174L..53M. doi:10.1086/180947.
Retrieved from "https://en.wikipedia.org/w/index.php?title=4U_1543-475&oldid=1149656927"