Detection of Intracluster Planetary Nebulae in the Coma Cluster

[OIII] lambda 5007AA emission lines of 16 intracluster planetary nebulae candidates in the Coma cluster were detected with a Multi-Slit Imaging Spectroscopy (MSIS) technique using FOCAS on the Subaru telescope. The identification of these faint emission sources as PNe is supported by (i) their point-like flux distribution in both space and wavelength, with tight limits on the continuum flux; (ii) the identification of the second [OIII] lambda 4959 line in the only object at high enough velocity that this line too falls into the filter bandpass; (iii) emission line fluxes consistent with PNe at... Mehr ...

Verfasser: Nobunari Kashikawa
Kenneth C. Freeman
Naoki Yasuda
Magda Arnaboldi
Sadanori Okamura
Ortwin Gerhard
Dokumenttyp: Artikel
Erscheinungsdatum: 2005
Schlagwörter: NEANIAS Space Research Community / Netherlands / Space and Planetary Science / Astronomy and Astrophysics
Sprache: Englisch
Permalink: https://search.fid-benelux.de/Record/base-29181545
Datenquelle: BASE; Originalkatalog
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Link(s) : https://www.openaccessrepository.it/record/98925

[OIII] lambda 5007AA emission lines of 16 intracluster planetary nebulae candidates in the Coma cluster were detected with a Multi-Slit Imaging Spectroscopy (MSIS) technique using FOCAS on the Subaru telescope. The identification of these faint emission sources as PNe is supported by (i) their point-like flux distribution in both space and wavelength, with tight limits on the continuum flux; (ii) the identification of the second [OIII] lambda 4959 line in the only object at high enough velocity that this line too falls into the filter bandpass; (iii) emission line fluxes consistent with PNe at 100 Mpc distance, in the range 2.8 x 10^