@booklet {41857,
	title = {A pulsating, possible type Ia supernova progenitor in the Large Magellanic},
	year = {2016},
	month = {2016/10/1},
	pages = {115},
	abstract = {We request a 50 ks observation of a pulsating (P~170 s), accretingwhite dwarf binary located in the Large Magellanic Cloud. The systemwas serendipitously detected off-axis during analysis of an archivalXMM-Newton observation (2013) that was severely contaminated by highbackground. Such objects are thought to be candidates for the progenitorsof type Ia supernovae, or may alternatively undergo accretion-inducedcollapse to form the neutron stars in some millisecond pulsars. Thenature of their short period oscillations remains unknown. The on-axisXMM-Newton observation proposed below would deliver a much improvedspectrum, allowing precise characterisation of the system.},
	url = {https://ui.adsabs.harvard.edu/abs/2016xmm..prop..115V},
	author = {Vasilopoulos, Georgios}
}
