Nova Scorpius 1437 A.D. is now a dwarf nova, age-dated by its proper motion

Abstract

Here we report the recovery of the binary underlying the classical nova of 11 March 1437 A.D. whose age is independently confirmed by proper motion-dating, and show that in the 20th century it exhibits dwarf nova eruptions. The four oldest recovered classical novae are now all dwarf novae. Taken together they strongly suggest that mass transfer rates decrease by an order of magnitude or more in the centuries after a classical nova event, greatly slowing the evolution, and lengthening the lifetimes of these explosive binary stars.

arXiv comment30 pages, 7 Figures

References in corpus (19)

• The Evolution of Cataclysmic Variables as Revealed by their Donor Stars
• An Extended Grid of Nova Models: II. The Parameter Space of Nova Outbursts
• First science with SALT: peering at the accreting polar caps of the eclipsing polar SDSS J015543.40+002807.2
• GASS: The Parkes Galactic All-Sky Survey. Update: improved correction for instrumental effects and new data release
• A catalogue of integrated H-alpha fluxes for 1,258 Galactic planetary nebulae
• BK Lyncis: The Oldest Old Nova?... And a Bellwether for Cataclysmic-Variable Evolution
• A remarkable recurrent nova in M31 - The optical observations
• Spectroscopy of two PN candidates in IC10
• Unveiling the nature of INTEGRAL objects through optical spectroscopy. X. A new multi-year, multi-observatory campaign
• AT Cnc: A Second Dwarf Nova with a Classical Nova Shell
• A remarkable recurrent nova in M31 - The X-ray observations
• The Behavior of Novae Light Curves Before Eruption
• High-resolution spectroscopy of the intermediate polar EX Hydrae. I. Kinematic study and Roche tomography
• When does an old nova become a dwarf nova? Kinematics and age of the nova shell of the dwarf nova AT Cnc
• Discovery of an eclipsing dwarf nova in the ancient nova shell Te 11
• The awakening of a classical nova from hibernation
• The Inter-Eruption Timescale of Classical Novae from Expansion of the Z Camelopardalis Shell
• The Bochum Survey of the Southern Galactic Disk: II. Follow-up measurements and multi-filter photometry for 1323 square degrees monitored in 2010-2015
• On the absence of nova shells

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• Cataclysmic variables as possible counterparts of ancient Far Eastern guest stars
• A new approach to generate a catalogue of potential historical novae
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• Introducing the Condor Array Telescope: III. The expansion and age of the shell of the dwarf nova Z Camelopardalis, and detection of a second, larger shell
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• Challenging historical novae: AT Cnc (1645), Te-11 (483), and M22 (BC 48) revisited
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