activity
19992026
most citedA PDR-Code Comparison Study

352 citations · 1.6k across the 43 of their papers we have counts for

collaborators
Showing astro-phShow all

6 papers · 1 filter

astro-ph2008★ 75 cited

The Evolution of NGC 7027 at Radio Frequencies: A New Determination of the Distance and Core Mass

Albert Zijlstra, P. A. M. van Hoof, R. A. Perley

We present the results of a 25-year program to monitor the radio flux evolution of the planetary nebula NGC7027. We find significant evolution of the spectral flux densities. The f…

astro-ph2007★ 352 cited

A PDR-Code Comparison Study

M. Roellig, N. P. Abel, T. Bell +21

We present a comparison between independent computer codes, modeling the physics and chemistry of interstellar photon dominated regions (PDRs). Our goal was to understand the mutua…

astro-ph2003★ 60 cited

Introducing EMILI: Computer Aided Emission Line Identification

Brian Sharpee, Robert Williams, Jack A. Baldwin +1

The identification of spectral lines can be a tedious process requiring the interrogation of large spectroscopic databases, but it does lend itself to software algorithms that can…

astro-ph2000

Properties of post-AGB stars with IRAS colors typical of planetary nebulae

Griet C. Van de Steene, Peter A. M. van Hoof, Peter R. Wood

We have investigated the infrared properties of a sample of objects with IRAS colors typical of planetary nebulae. The selected objects have not yet evolved to the planetary nebula…

astro-ph1999★ 27 cited

Measuring angular diameters of extended sources

P. A. M. van Hoof

When measuring diameters of partially resolved sources often a technique called gaussian deconvolution is used. This technique yields a gaussian diameter which subsequently has to…

astro-ph1999★ 30 cited

Properties of Dust Grains in Planetary Nebulae -- I. The Ionized Region of NGC 6445

P. A. M. van Hoof, G. C. Van de Steene, D. A. Beintema +3

In this paper we study new infrared spectra of the evolved planetary nebula NGC 6445 obtained with ISO. These data show that the thermal emission from the grains is very cool and h…