<?xml version="1.0" encoding="UTF-8"?><xml><records><record><source-app name="Biblio" version="7.x">Drupal-Biblio</source-app><ref-type>17</ref-type><contributors><authors><author><style face="normal" font="default" size="100%">Reig, P.</style></author><author><style face="normal" font="default" size="100%">Primak, N.</style></author><author><style face="normal" font="default" size="100%">Akras, S.</style></author><author><style face="normal" font="default" size="100%">Hatzidimitriou, D.</style></author><author><style face="normal" font="default" size="100%">Pietsch, W.</style></author><author><style face="normal" font="default" size="100%">Papamastorakis, G.</style></author></authors></contributors><titles><title><style face="normal" font="default" size="100%">Optical spectra of Nova 2008-06b</style></title><short-title><style face="normal" font="default" size="100%">The Astronomer's Telegram</style></short-title></titles><keywords><keyword><style  face="normal" font="default" size="100%">Novae</style></keyword><keyword><style  face="normal" font="default" size="100%">Optical</style></keyword></keywords><dates><year><style  face="normal" font="default" size="100%">2008</style></year><pub-dates><date><style  face="normal" font="default" size="100%">2008/07/1</style></date></pub-dates></dates><urls><web-urls><url><style face="normal" font="default" size="100%">https://ui.adsabs.harvard.edu/abs/2008ATel.1612....1R</style></url></web-urls></urls><volume><style face="normal" font="default" size="100%">1612</style></volume><pages><style face="normal" font="default" size="100%">1</style></pages><language><style face="normal" font="default" size="100%">eng</style></language><abstract><style face="normal" font="default" size="100%">We carried out spectroscopic observations of the optical transient near M31 reported in ATel #1591 (RA = 0h42m27s.81 DEC =+41o14'48&quot;.2 (J2000)) from the 1.3m telescope of the Skinakas Observatory in Crete (Greece) on the nights 27 June 2008 and 2 July 2008. The spectra covered the range 5080-7160 angstroms. The Halpha appeared strongly in emission and displayed a double peaked profile. The ratio of the blue peak to the red peak (B/R) reversed from B &amp;gt; R (i.e blue-dominated profile) on 27 June to B &amp;lt; R (i.e red-dominated profile) on 2 July.</style></abstract></record></records></xml>