| 词条 | T Boötis |
| 释义 |
Despite being usually referred to as a nova, it had characteristics that set it apart from other novae - an amplitude of at least 7 magnitudes, an unusually rapid decline in brightness and a location unusually far from the Galactic plane.[3] Joseph Ashbrook suggested in 1953 that it may be a recurrent nova which has been observed only once.[4] References1. ^1 2 3 {{cite web|title=VSX: Detail for T Boo|url=http://www.aavso.org/vsx/index.php?view=detail.top&oid=4306|website=The International Variable Star Index|publisher=AAVSO|accessdate=16 May 2015|archiveurl=https://www.webcitation.org/6YYmz24nj|archivedate=16 May 2015}} {{Stars of Boötes}}{{DEFAULTSORT:T Bootis}}{{var-star-stub}}2. ^1 {{cite web|last1=Baxendell|first1=Joseph|title=On the Three New Variable Stars, T Bootis, T. Serpentis, and S Delphini|url=http://adsabs.harvard.edu/full/1861MNRAS..21...68B|website=SAO/NASA Astrophysics Data System (ADS)|publisher=Smithsonian Astrophysical Observatory|accessdate=16 May 2015|archiveurl=https://www.webcitation.org/6YYbOnRR3|archivedate=16 May 2015}} 3. ^1 {{cite book|last1=Burnham|first1=Robert|title=Burnham's Celestial Handbook Volume 1|date=1978|publisher=Dover|isbn=0-486-23567-X|page=311|url=https://books.google.com.au/books?id=z3_CAgAAQBAJ&pg=PA311&dq=t+bootis+celestial+handbook&hl=en&sa=X&ei=gKdWVeWmFuKzmwXJxYHABA&ved=0CBwQ6AEwAA#v=onepage&q=t%20bootis%20celestial%20handbook&f=false|accessdate=16 May 2015}} 4. ^{{cite web|last1=Ashbrook|first1=Joseph|title=Notes on Four Novae|url=http://adsabs.harvard.edu/full/1953AJ.....58..175F|website=SAO/NASA Astrophysics Data System (ADS)|publisher=Smithsonian Astrophysical Observatory|accessdate=16 May 2015|archiveurl=https://www.webcitation.org/6YYkHUYgs|archivedate=16 May 2015}} 4 : Novae|Boötes|1860 in science|Objects with variable star designations |
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