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View Full Version here: : Possible nova in Oph PNV J17144255-2943481


Jon
13-04-2014, 11:16 PM
Here's the CBAT page (http://www.cbat.eps.harvard.edu/unconf/followups/J17144255-2943481.html) - discovered a couple of days ago.

I got a low-res SA100 spectrum last night. Strong blue continuum. Odd sort of line profile - weak Ha emission line, no sign of Hb, but a stronger He/N(?) emission line around 4680. Possibly a He/N type nova close to maximum?

Rob_K
13-04-2014, 11:54 PM
Nice work Jon! My guess is that it's a dwarf nova of some sort, very blue. Check these out:
http://www.galaxyzooforum.org/index.php?topic=276258.15

My shot last night showed no sign of reddening at all - a classical nova of this magnitude and in that position should appear reddish in my shots. That is, at mag 10.3-odd, it has to be either a long way away and/or subject to extinction due to dust. Either (both!) would produce a reddish object in that position. Therefore it must be this side of the dust and not as intrinsically bright as a classical nova - ie a dwarf nova or some other cv. Or not LOL!

Edit - very similar to the recent PNV in Hercules, now confirmed as a dwarf nova, with superhumps. Spectrum here:
http://quasar.teoth.it/html/spectra/PNVJ17592412+2520317.jpg

Cheers -

Jon
14-04-2014, 12:28 AM
Agreed, Rob. It doesn't feel quite right. I'm not 100% convinced that the "line" at 4680 isn't a field star. Trying again as I write.

The Ha is real. But that could be a lot of things.

Rob_K
14-04-2014, 12:41 AM
Yep, that's H-alpha but any redness is swamped by the strong blue continuum. Gotta be a dwarf nova!

Cheers -

Rob_K
14-04-2014, 02:20 PM
Another spectrum has been posted and the object identified as a dwarf nova:
http://ooruri.kusastro.kyoto-u.ac.jp/mailarchive/vsnet-alert/17217
http://otobs.org/FBO/etc/pnv_j17144255-2943481_20140413.png

Cheers -

Jon
14-04-2014, 06:07 PM
Good to see Fujii-san's spectrum also catches the emission band at 4680. Wasn't my imagination.