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Wikipedia:Peer review/Caelum/archive1

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This peer review discussion has been closed.
I've listed this article for peer review because I think it is quite close to FA-standard, but to be honest, the article is quite short, and I was wondering if there was anything that I was missing, or if there are other problems present.

Thanks, StringTheory11 (t • c) 03:46, 27 February 2014 (UTC)[reply]

Comment: it's a brief article but covers the topic reasonably well and is decent shape. Here's a few observations:

  • There's a number of instances of redundant wording: 'also', 'another'.
  • "a rather nearby"; vague
  • "that at first appeared to contain a jet but no host galaxy"; this wording is a little unclear
  • "the system will likely become a cataclysmic variable star due to the period's gradual shortening"; I think this could be explained a little better. For example, here's what it says in the paper: "The continued loss of angular momentum will shrink the Roche lobe of the M-dwarf to the point where mass transfer will start from the M-dwarf to the white dwarf through the inner Lagrangian point. RR Cae will then be a cataclysmic variable star."
  • "there is evidence for a second hypothetical substellar body"; evidence for a hypothetical body? Is this just redundancy or something else?
  • "Ridpath, Ian; Wil Tirion"; the second name is in an inconsistent format.
  • It's difficult to see in the north, so you could list the lowest northern latitude where this constellation can not be viewed.

Unfortunately, I couldn't find anything else to add. Hopefully these comments are of some use. Praemonitus (talk) 02:53, 13 March 2014 (UTC)[reply]

Thank you! StringTheory11 (t • c) 02:21, 15 March 2014 (UTC)[reply]
You're welcome. Praemonitus (talk) 19:43, 17 March 2014 (UTC)[reply]