Stellar Multiplicity of M Dwarfs with Short-period Giant Planets, and the Characterization of TOI-5628Ab, Gan, Tianjun, L’Heureux, Alexandrine, Cadieux, Charles, Mao, Shude, Pallé, Enric, Wang, Sharon X., Stassun, Keivan G., Howell, Steve B., Rackham, Benjamin V., Grondin, Steffani M., Barkaoui, Khalid, Arnold, Luc, Artigau, Étienne, Burdanov, Artem, Burgasser, Adam J., Caldwell, Douglas A., Ciardi, David R., Collins, Karen A., Cook, Neil J., Doyon, René, Dransfield, Georgina, Fukui, Akihiko, Gillon, Michaël, Jehin, Emmanuel, Murgas, Felipe, Narita, Norio, Noguer, Federico R., Relles, Howard M., Shporer, Avi, Simon, Molly N., Soubkiou, Abderahmane, Theissen, Christopher A., Timmermans, Mathilde, Triaud, Amaury H. M. J., Zellem, Robert T., Zúñiga-Fernández, S., Machado, Celso P., Mason, Ian R., Mazzucato, Michele T., Zhao, Jingyuan

A recent study finds that a recurrent nova may be powered by a rare Be star–white dwarf binary system, broadening the scope of possible novae origins.

ATel On

Discovery of Two New Eruptions of the Ultrashort Recurrence Time Nova M31N 2017-01e* , Allen W. Shafter, Jingyuan Zhao, Kamil Hornoch, Hana Kučáková, Kenta Taguchi, Jiashuo Zhang, Jia You, Binyu Wang, Runwei Xu, Weiye Wang, Yuqing Ren, Lanhe Ding, Xiaochang Yan, Mi Zhang, Wei-Hao Wang, Howard E. Bond, Robert Williams, Gregory R. Zeimann

A new brightness forecast for Comet Tsuchinshan-ATLAS whets our hopes for a fine appearance in late September and early October.

With T Coronae Borealis soon rising to naked-eye visibility, recurrent novae are in the news. Recurrent nova M31N 2008-12a is the subject of today's article.