activity
20032009
most citedThe N2D+/N2H+ ratio as an evolutionary tracer of Class 0 protostars

159 citations · 230 across the 4 of their papers we have counts for

collaborators

7 papers

astro-ph.GA200916 cited

The molecular environment of the massive star forming region NGC 2024: Multi CO transition analysis

M. Emprechtinger, M. C. Wiedner, R. Simon +10

NGC 2024, a sites of massive star formation, have complex internal structures caused by cal heating by young stars, outflows, and stellar winds. These complex cloud structures lead…

astro-ph2008159 cited

The N2D+/N2H+ ratio as an evolutionary tracer of Class 0 protostars

M. Emprechtinger, P. Caselli, N. H. Volgenau +2

Deuterated ions are abundant in cold (T=10 K), dense (n=10^5 cm^-3) regions, in which CO is frozen out onto dust grains. In such environments, the deuterium fractionation of such i…

astro-ph200640 cited

First observations with CONDOR, a 1.5 THz heterodyne receiver

M. C. Wiedner, G. Wieching, F. Bielau +15

The THz atmospheric windows centered at roughly 1.3 and 1.5~THz, contain numerous spectral lines of astronomical importance, including three high-J CO lines, the N+ line at 205 mic…

astro-ph200615 cited

Probable detection of H2D+ in the starless core Barnard 68

M. R. Hogerheijde, P. Caselli, M. Emprechtinger +8

The presence of H2D+ in dense cloud cores underlies ion-molecule reactions that strongly enhance the deuterium fractionation of many molecular species. We determine the H2D+ abunda…

astro-ph2004

Photoionization models of roundish galactic planetary nebulae in the thick disk

M. Emprechtinger, T. Rauch, S. Kimeswenger

We present the result of photo-ionizing modelling of the three planetary nebulae (PNe) A 20, A 15 and MeWe 1-3. All three objects are roughly roundish, highly excited and have a hi…

astro-ph2004

Spectroscopic investigation of unstudied southern PNe

M. Emprechtinger, T. Forveille, S. Kimeswenger

We present a spectroscopic investigation of two hitherto unstudied galactic planetary nebulae (MeWe 1-10 and MeWe 1-11) and one candidate object (MeWe 2-5). The candidate object cl…