New upper limit on intensity of forbidden Fe XIV 5303 in Tycho's supernova remnant

Details New upper limit on intensity of forbidden Fe XIV 5303 in Tycho's supernova remnant New upper limit on intensity of forbidden Fe XIV 5303 in Tycho's supernova remnant

Oct 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990apj...362..563t&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 362, Oct. 20, 1990, p. 563-565.

Astronomy and Astrophysics

Astrophysics

2

Charge Coupled Devices, Emission Spectra, Iron, Supernova Remnants, Light Curve, Stellar Mass Ejection, White Dwarf Stars

Scientific paper

Analysis of a CCD image of the remnant of Tycho's supernova made in the forbidden coronal green line fails to reveal emission at a limit of 3.1 x 10 to the -8th ergs/sq cm s sr at the location of the reverse shock into the ejecta. The nondetection may imply that the reverse shock has not yet reached Fe-enriched ejecta or that the known clumpiness of the ejecta prevents production of observable amounts of Fe(+13).

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