HD 168607: Perbedaan antara revisi
Konten dihapus Konten ditambahkan
Telah ditambahkan ke kategori Tag: Suntingan perangkat seluler Suntingan peramban seluler Suntingan seluler lanjutan |
Rescuing 3 sources and tagging 0 as dead.) #IABot (v2.0.9.5 |
||
(3 revisi perantara oleh 3 pengguna tidak ditampilkan) | |||
Baris 1:
{{Starbox begin|name=HD 168607}}
{{Starbox observe|epoch=J2000|ra={{RA|18|21|14.889}}<ref name=hipparcos>{{cite journal|bibcode=2007A&A...474..653V|title=Validation of the new Hipparcos reduction|journal=Astronomy and Astrophysics|volume=474|issue=2|pages=653|author1=Van Leeuwen|first1=F.|year=2007|doi=10.1051/0004-6361:20078357|arxiv = 0708.1752 }}</ref>|dec={{DEC|-16|22|31.76}}<ref name=hipparcos/>|appmag_v=8.28<ref name=ducati>{{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|pages=0|author1=Ducati|first1=J. R.|year=2002}}</ref> (var)|constell=[[Sagittarius (constellation)|Sagittarius]]}}
{{Starbox character|class=B9Ia<sup>+</sup><ref name=chentsov>{{cite journal|last1=Chentsov|first1=E. L.|last2=Ermakov|first2=S. V.|last3=Klochkova|first3=V. G.|last4=Panchuk|first4=V. E.|last5=Bjorkman|first5=K. S.|last6=Miroshnichenko|first6=A. S.|title=An atlas of spectra of B6-A2 hypergiants and supergiants from 4800 to 6700Å|journal=Astronomy and Astrophysics|volume=397|issue=3|year=2003|pages=1035–1042|doi=10.1051/0004-6361:20021430|bibcode=2003A&A...397.1035C|url=http://libres.uncg.edu/ir/uncg/f/A_Miroshnichenko_AnAtlasofSpectra_2003.pdf|access-date=2020-08-21|archive-date=2019-04-27|archive-url=https://web.archive.org/web/20190427142209/http://libres.uncg.edu/ir/uncg/f/A_Miroshnichenko_AnAtlasofSpectra_2003.pdf|dead-url=no}}</ref>|b-v=1.54<ref name=ducati/>|u-b=0.41<ref name=ducati/>|j-k=1.06<ref name=ducati/>|variable=[[Luminous blue variable|LBV]]<ref name=naze>{{cite journal|bibcode=2012A&A...538A..47N|title=The first X-ray survey of Galactic luminous blue variables|journal=Astronomy & Astrophysics|volume=538|pages=A47|author1=Nazé|first1=Y.|last2=Rauw|first2=G.|last3=Hutsemékers|first3=D.|year=2012|doi=10.1051/0004-6361/201118040|arxiv = 1111.6375 }}</ref>}}
{{Starbox astrometry|radial_v=-30<ref>{{cite journal|bibcode=2007AN....328..889K|title=Astrophysical supplements to the ASCC-2.5: Ia. Radial velocities of ˜55000 stars and mean radial velocities of 516 Galactic open clusters and associations|journal=Astronomische Nachrichten|volume=328|issue=9|pages=889|author1=Kharchenko|first1=N. V.|last2=Scholz|first2=R.-D.|last3=Piskunov|first3=A. E.|last4=Röser|first4=S.|last5=Schilbach|first5=E.|year=2007|doi=10.1002/asna.200710776|arxiv = 0705.0878 }}</ref>|prop_mo_ra=-0.27<ref name=hipparcos/>|prop_mo_dec=-1.01<ref name=hipparcos/>|parallax=1.85|p_error=1.29|parallax_footnote=<ref name=hipparcos/>|absmag_v=
{{Starbox detail|luminosity=240,000<ref name=variable/>|temperature=9,300<ref name=variable/>|gravity=1.0<ref name=variable/>}}
{{Starbox catalog|names=[[Variable star designation|V4029]] Sgr, [[Henry Draper catalogue|HD ]] 168607, [[Bonner Durchmusterung|BD ]]-16°4829, [[Smithsonian Astrophysical Observatory Star Catalog|SAO ]]161374, [[Hipparcos catalogue|HIP ]]89956, [[AAVSO]] 1815-16}}
Baris 11:
== Properti ==
HD 168607 biasanya diasumsikan berada pada jarak yang sama dari Nebula Omega (2,2 kilo parsec, 7.200 tahun cahaya, dari Matahari) dan secara fisik dapat dikaitkan dengan [[HD 168625]].<ref name="Chentsov 461–468">{{Cite journal|last=Chentsov|first=E. L.|last2=Gorda|first2=E. S.|date=2004-07|title=Spatial closeness of the white hypergiants HD 168607 and HD 168625|url=http://dx.doi.org/10.1134/1.1774398|journal=Astronomy Letters|volume=30|issue=7|pages=461–468|doi=10.1134/1.1774398|issn=1063-7737|access-date=2020-08-21|archive-date=2023-08-12|archive-url=https://web.archive.org/web/20230812103717/https://link.springer.com/article/10.1134/1.1774398|dead-url=no}}</ref> Dengan asumsi jarak ini benar, bintang ini<ref name="van Genderen 508–531">{{Cite journal|last=van Genderen|first=A. M.|date=2001-02|title=S Doradus variables in the Galaxy and the Magellanic Clouds|url=http://dx.doi.org/10.1051/0004-6361:20000022|journal=Astronomy & Astrophysics|volume=366|issue=2|pages=508–531|doi=10.1051/0004-6361:20000022|issn=0004-6361|access-date=2020-08-21|archive-date=2023-08-12|archive-url=https://web.archive.org/web/20230812103730/https://www.aanda.org/articles/aa/abs/2001/05/aads1896/aads1896.html|dead-url=no}}</ref> memiliki luminositas 240.000 kali lebih terang dari Matahari dengan suhu permukaan dari 9300 K.<ref
== Referensi ==
[[Kategori:Sagittarius]]
[[Kategori:
[[Kategori:
[[Kategori:
[[Kategori:
[[Kategori:Objek Durchmusterung]]
|