The recovery of CK Vulpeculae /Nova 1670/ - The oldest 'old nova'

Details The recovery of CK Vulpeculae /Nova 1670/ - The oldest 'old nova' The recovery of CK Vulpeculae /Nova 1670/ - The oldest 'old nova'

Jul 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982apj...258l..41s&link_type=abstract

Astrophysical Journal, Part 2 - Letters to the Editor, vol. 258, July 1, 1982, p. L41-L44.

Other

28

Interstellar Matter, Nebulae, Novae, Stellar Evolution, Stellar Mass Ejection, Stellar Radiation, Stellar Spectrophotometry, White Dwarf Stars

Scientific paper

Comparison of narrow-band H-alpha with continuum plates has yielded the location of CK Vulpeculae, a slow nova which reached-maximum brightness of about three in 1670 and again in 1671. CK Vul affords us the opportunity to study a nova remnant almost two centuries older than any other known. Associated with the central object are two nebulous blobs radiating mostly H-alpha and forbidden N II. These nebulae are probably ejecta of the nova sweeping up interstellar matter.

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