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astro-ph.SR2016
SU Lyncis, a hard X-ray bright M giant: Clues point to a large hidden population of symbiotic stars
K. Mukai, G. J. M. Luna, G. Cusumano +6
Symbiotic star surveys have traditionally relied almost exclusively on low resolution optical spectroscopy. However, we can obtain a more reliable estimate of their total Galactic…
astro-ph.SR2016
Photometric evolution of the 2016 outburst of recurrent Nova LMC 1968: the first three weeks
U. Munari, F. M. Walter, F. -J. Hambsch +1
Optical (BVRI) photometry of the first three weeks of the 2016 outburst of the recurrent Nova LMC 1968 is presented and discussed. The 2016 I-band light-curve is an exact replica,…
astro-ph.SR2016
The 2015 super-active state of recurrent nova T CrB and the long term evolution after the 1946 outburst
U. Munari, S. Dallaporta, G. Cherini
The recurrent nova T CrB has entered in 2015 a phase of unprecedented high activity. To trace something equivalent, it is necessary to go back to 1938, before the last nova eruptio…