CE Gruis: Difference between revisions
Content deleted Content added
Tom.Reding (talk | contribs) m →top: WL 1 first-publisher; WP:GenFixes on; using AWB |
Use {{cite simbad}} |
||
| Line 3: | Line 3: | ||
|name= CE Gruis |
|name= CE Gruis |
||
|type= |
|type= |
||
|ra= {{RA|21|37|56.38}} |
|ra= {{RA|21|37|56.38}}<ref name=SIMBAD>{{cite simbad |title = V* CE Gru |accessdate = 10 February 2014}}</ref> |
||
|dec= {{DEC|-43|42|13.1}} |
|dec= {{DEC|-43|42|13.1}}<ref name=SIMBAD/> |
||
}} |
}} |
||
'''CE Gruis''' is a (also known as '''Grus V-1''') is a faint (magnitude 18–21) binary star system in the [[constellation]] [[Grus (constellation)|Grus]]. It is composed of a [[white dwarf]] and donor star, in this case the two are so close and fused into orbit facing one another. Known as [[Polar (cataclysmic variable star)|polars]], material from the donor star does not form an accretion disc around the white dwarf, but rather streams directly onto it.<ref name="ramsay02">{{cite journal|author1=Ramsay, Gavin |author2=Cropper, Mark |year=2002|title=First X-ray Observations of the Polar CE Gru|journal=Monthly Notices of the Royal Astronomical Society|volume=335|issue=4|pages=918–22|url=http://articles.adsabs.harvard.edu/cgi-bin/nph-iarticle_query?2002MNRAS.335..918R&data_type=PDF_HIGH&whole_paper=YES&type=PRINTER&filetype=.pdf |bibcode=2002MNRAS.335..918R|arxiv = astro-ph/0205102 |doi = 10.1046/j.1365-8711.2002.05666.x }}</ref> |
'''CE Gruis''' is a (also known as '''Grus V-1''') is a faint (magnitude 18–21) binary star system in the [[constellation]] [[Grus (constellation)|Grus]]. It is composed of a [[white dwarf]] and donor star, in this case the two are so close and fused into orbit facing one another. Known as [[Polar (cataclysmic variable star)|polars]], material from the donor star does not form an accretion disc around the white dwarf, but rather streams directly onto it.<ref name="ramsay02">{{cite journal|author1=Ramsay, Gavin |author2=Cropper, Mark |year=2002|title=First X-ray Observations of the Polar CE Gru|journal=Monthly Notices of the Royal Astronomical Society|volume=335|issue=4|pages=918–22|url=http://articles.adsabs.harvard.edu/cgi-bin/nph-iarticle_query?2002MNRAS.335..918R&data_type=PDF_HIGH&whole_paper=YES&type=PRINTER&filetype=.pdf |bibcode=2002MNRAS.335..918R|arxiv = astro-ph/0205102 |doi = 10.1046/j.1365-8711.2002.05666.x }}</ref> |
||
| Line 17: | Line 17: | ||
[[Category:Polars (cataclysmic variable stars)]] |
[[Category:Polars (cataclysmic variable stars)]] |
||
[[Category:Objects with variable star designations|Gruis, CE]] |
[[Category:Objects with variable star designations|Gruis, CE]] |
||
{{multi-star-stub}} |
|||
{{var-star-stub}} |
|||
Revision as of 19:05, 16 March 2018
| Observation data Epoch J2000.0 Equinox J2000.0 (ICRS) | |
|---|---|
| Constellation | Grus |
| Right ascension | 21h 37m 56.38s[1] |
| Declination | −43° 42′ 13.1″[1] |
CE Gruis is a (also known as Grus V-1) is a faint (magnitude 18–21) binary star system in the constellation Grus. It is composed of a white dwarf and donor star, in this case the two are so close and fused into orbit facing one another. Known as polars, material from the donor star does not form an accretion disc around the white dwarf, but rather streams directly onto it.[2]
References
- ^ a b "V* CE Gru". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 10 February 2014.
- ^ Ramsay, Gavin; Cropper, Mark (2002). "First X-ray Observations of the Polar CE Gru" (PDF). Monthly Notices of the Royal Astronomical Society. 335 (4): 918–22. arXiv:astro-ph/0205102. Bibcode:2002MNRAS.335..918R. doi:10.1046/j.1365-8711.2002.05666.x.
{{cite journal}}: CS1 maint: unflagged free DOI (link)
 | This binary or multiple star system–related article is a stub. You can help Wikipedia by expanding it. |
 | This variable star–related article is a stub. You can help Wikipedia by expanding it. |