activity
20102015
most citedChemical abundances and properties of the ionized gas in NGC 1705

27 citations · 27 across the 1 of their papers we have counts for

collaborators

6 papers

astro-ph.GA2015★ 27 cited

Chemical abundances and properties of the ionized gas in NGC 1705

F. Annibali, M. Tosi, A. Pasquali +3

We obtained [O III] narrow-band imaging and multi-slit MXU spectroscopy of the blue compact dwarf (BCD) galaxy NGC 1705 with FORS2@VLT to derive chemical abundances of PNe and H II…

astro-ph.HE2013

A disrupted bulgeless satellite galaxy as counterpart of the ultraluminous X-ray source ESO 243-49 HLX-1

M. Mapelli, F. Annibali, L. Zampieri +1

The point-like X-ray source HLX-1, close to the S0 galaxy ESO 243-49, is one the strongest intermediate-mass black hole candidates, but the nature of its counterpart is still puzzl…

astro-ph.CO2013

A minor merger scenario for the ultraluminous X-ray source ESO 243-49 HLX-1 - II. Constraints from photometry

M. Mapelli, F. Annibali, L. Zampieri +1

The point-like X-ray source HLX-1, close to the S0 galaxy ESO 243-49, is the brightest known ultraluminous X-ray source and one the strongest intermediate-mass black hole candidate…

astro-ph.HE2012

A minor merger scenario for the ultraluminous X-ray source ESO 243-49 HLX-1

M. Mapelli, L. Zampieri, L. Mayer

The point-like X-ray source HLX-1 is the brightest known ultraluminous X-ray source and likely the strongest intermediate-mass black hole candidate. HLX-1 is hosted in the S0 galax…

astro-ph.CO2010

Nature and nurture of early-type dwarf galaxies in low density environments

R. Grützbauch, F. Annibali, R. Rampazzo +2

We study stellar population parameters of a sample of 13 dwarf galaxies located in poor groups of galaxies using high resolution spectra observed with VIMOS at the ESO-VLT. LICK-in…

astro-ph.CO2010

Nearby early-type galaxies with ionized gas VI. The Spitzer-IRS view

P. Panuzzo, R. Rampazzo, A. Bressan +5

We present low resolution Spitzer-IRS spectra of 40 ETGs, selected from a sample of 65 ETGs showing emission lines in their optical spectra. We homogeneously extract the mid-infrar…