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19992006
most citedThe distribution of the ISM in the Milky Way A three-dimensional large-scale model

138 citations · 138 across the 2 of their papers we have counts for

collaborators

9 papers

astro-ph2006138 cited

The distribution of the ISM in the Milky Way A three-dimensional large-scale model

A. Misiriotis, E. M. Xilouris, J. Papamastorakis +2

We use the COBE/DIRBE (1.2, 2.2, 60, 100, 140, and 240 m) maps and the COBE/FIRAS spectra (for the wavelength range 100 - 1000 m) to constrain a model for the spatial distrib…

astro-ph2006

New Planerary Nebulae towards the Galactic bulge

P. Boumis, S. Akras, P. A. M. van Hoof +3

New Planetary Nebulae (PNe) were discovered through an [O III] 5007 A emission line survey in the Galactic bulge region with l>0 deg. We detected 240 objects, including 44 new PNe.…

astro-ph2006

New Planetary Nebulae in the Galactic Bulge region with l>0deg - II

P. Boumis, S. Akras, E. M. Xilouris +4

The presentation of new results from an [O III] 5007 A survey in a search for planetary nebulae (PNe) in the galactic bulge is continued. A total of 60 objects, including 19 new PN…

astro-ph2005

B and I-band optical micro-variability observations of the BL Lac objects S5 2007+777 and 3C371

E. M. Xilouris, I. E. Papadakis, P. Boumis +5

We have observed S5 2007+777 and 3C371 in the B and I bands for 13 and 8 nights, respectively, during various observing runs in 2001, 2002 and 2004. The observations resulted in al…

astro-ph2005

The faint supernova remnant G 116.5+1.1 and the detection of a new candidate remnant

F. Mavromatakis, P. Boumis, E. M. Xilouris +2

The extended supernova remnant G 116.5+1.1 was observed in the optical emission lines of Halpha+[N II], [S II] and [O III]; deep long-slit spectra were also obtained. The morpholog…

astro-ph2003

Dust masses and star formation in bright IRAS galaxies Application of a physical model for the interpretation of FIR observations

A. Misiriotis, I. E. Papadakis, N. D. Kylafis +1

We address the problem of modeling the far-infrared (FIR) spectrum and deriving the star-formation rate (SFR) and the dust mass of spiral galaxies. We use the realistic physical mo…