F06296$+$5743 : A Very Massive Starburster ?

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dc.creatorHuang, J. H.
dc.creatorGu, Q. S.
dc.creatorSu, H. J.
dc.creatorShang, Z. H.
dc.date1996-04-11
dc.date.accessioned2026-07-07T02:21:07Z
dc.date.available2026-07-07T02:21:07Z
dc.descriptionWe have observed an object having strong Balmer absorption lines and blue continuum. The inference about the nuclear stellar population drawn from the line ratios is basically coincident with that drawn from the continuum color, both indicating the dominant fraction of early A type population in the nucleus. This might be expected only if there has been a very massive starburst, burst strength of $>$ 10\% at least.
dc.description4 pages, l-aa.sty, 1 figure available on request at jhh@nju.edu.cn, accepted for publication in A\&A
dc.identifierhttps://arxiv.org/abs/astro-ph/9604058
dc.identifierhttp://arxiv.org/abs/astro-ph/9604058
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/10434
dc.subjectAstrophysics
dc.titleF06296$+$5743 : A Very Massive Starburster ?
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