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Post Info TOPIC: SDSS J144011.01+494733.4


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Posts: 131433
Date:
CSS090530:144011+494734
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Title: CSS090530:144011+494734: a new SU UMa-type dwarf nova in Bootes
Authors: David Boyd, Nick Dunckel, Jerry Foote, Ian Miller
(Version v2)

We report photometry and analysis of a previously unknown SU UMa-type dwarf nova in Bootes detected in outburst by the Catalina Real-time Transient Survey on 2009 May 30 with the discovery identifier CSS090530:144011+494734. This apparently stellar object had previously been catalogued by the Sloan Digital Sky survey as SDSS J144011.01+494733.4. We measured its mean superhump period over the first 3 days following detection as 0.06500(4) d at which point this changed to 0.06438(3) d. We detected a possible orbital period of 0.06322(8) d implying a mean superhump period excess of 0.020(2). After detection, the dwarf nova maintained steady brightness for 5 days before starting to fade. The outburst amplitude was 5.5 magnitudes above its quiescent level.

Read more (276kb, PDF)

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L

Posts: 131433
Date:
SDSS J144011.01+494733.4
Permalink  
 


Title: SDSS J144011.01+494733.4: a new SU UMa-type dwarf nova in Bootes
Authors: David Boyd, Nick Dunckel, Jerry Foote, Ian Miller

We report photometry and analysis of a previously unknown SU UMa-type dwarf nova in Bootes detected in outburst by the Catalina Real-time Transient Survey on 2009 May 30 with the event identifier CSS090530:144011+494734. This apparently stellar object had previously been catalogued by the Sloan Digital Sky survey as SDSS J144011.01+494733.4. We measured its mean superhump period over the first 3 days following detection as 0.06500(4) d at which point this changed to 0.06438(3) d. We detected a possible orbital period of 0.06322(8) d implying a mean superhump period excess of 0.020(2). After detection, the dwarf nova maintained steady brightness for 5 days before starting to fade. The outburst amplitude was 5.5 magnitudes above its quiescent level.

Read more (277kb, PDF)

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