UBV photometry of Markarian and S0 galaxies

Peterson, B. M.; Fricke, K. J.; Biermann, Peter L.

doi:10.1086/130823

Cited by 3 publications

(4 citation statements)

References 4 publications

(12 reference statements)

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“…8), however, shows narrow (FWHM < 280 kms −1 ) emission lines with λ6584/Hα = 0.16; this object is therefore a HII region. A λ6300 emission line is observed with λ6300/Hα = 0.015 Mark 469, CG 899 (Pesch & Sanduleak, 1989) or KUG 1416+345 (Takase & Miyauchi-Isobe, 1984) is a 16.1 mag, UV excess galaxy (Peterson et al, 1981). Our observations (Fig.…”

Section: Notes On Individual Objectssupporting

confidence: 50%

“…A λ6300 emission line is observed with λ6300/Hα = 0.015. Mark 469, CG 899 (Pesch & Sanduleak 1989) or KUG 1416+345 (Takase & Miyauchi-Isobe 1984) is a 16.1 mag, UV excess galaxy (Peterson et al 1981). Our observations (Fig.…”

Section: Observationsmentioning

confidence: 51%

“…This object is, therefore, a HII region. Mark 483 = CG 741 (Sanduleak & Pesch 1987) is an emission line galaxy (Markarian et al 1988;Izotov et al 1993) with a strong UV excess (U − B = −0.45, Peterson et al 1981). The emission-line ratios published by Markarian et al (λ6584/Hα < 0.33) and Izotov et al (λ5007/Hβ ∼ 2.0) suggested that it is a HII region.…”

Section: Observationsmentioning

confidence: 98%

“…Mark 483 = CG 741 (Sanduleak & Pesch, 1987) is an emission line galaxy (Markarian et al, 1988;Izotov et al, 1993) with a strong UV excess (U-B = −0.45, Peterson et al, 1981) 2.0) suggested that it is a HII region. This is confirmed by our spectrum (Fig.…”

Section: Notes On Individual Objectsmentioning

confidence: 99%

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