Materials Map

Discover the materials research landscape. Find experts, partners, networks.

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The Materials Map is an open tool for improving networking and interdisciplinary exchange within materials research. It enables cross-database search for cooperation and network partners and discovering of the research landscape.

The dashboard provides detailed information about the selected scientist, e.g. publications. The dashboard can be filtered and shows the relationship to co-authors in different diagrams. In addition, a link is provided to find contact information.

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Materials Map under construction

The Materials Map is still under development. In its current state, it is only based on one single data source and, thus, incomplete and contains duplicates. We are working on incorporating new open data sources like ORCID to improve the quality and the timeliness of our data. We will update Materials Map as soon as possible and kindly ask for your patience.

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693.932 PEOPLE
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Naji, M.
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Zijlstra, Albert

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in Cooperation with on an Cooperation-Score of 37%

Topics

Publications (15/15 displayed)

  • 2023The heart of Sakurai's Object revealed by ALMA4citations
  • 2021Dust Formation in a Primitive Environmentcitations
  • 2021Dust Formation in a Primitive Environmentcitations
  • 2020The infrared view of dust and molecules around V4334 Sgr (Sakurai’s Object): a 20-year retrospective21citations
  • 2019Stellar Pulsation and the Production of Dust and Molecules in Galactic Carbon Stars9citations
  • 2016The Infrared Spectral Properties of Magellanic Carbon Stars48citations
  • 2016The Infrared Spectral Properties of Magellanic Carbon Stars48citations
  • 2014The Herschel planetary nebula survey (HerPlaNS): I. Data overview and analysis demonstration with NGC? 678134citations
  • 2011The identification of probable SiS emission at 13-14 μm in spectra of galactic S stars9citations
  • 2009Unusual dust emission from planetary nebulae in the magellanic clouds81citations
  • 2008The Magellanic zoo: Mid-infrared Spitzer spectroscopy of evolved stars and circumstellar dust in the Magellanic Clouds100citations
  • 2007Luminosities and mass-loss rates of carbon stars in the Magellanic Clouds101citations
  • 2007Molecules and dust grains in AGB stars in nearby galaxies - The influence of metallicitiescitations
  • 2006A Spitzer mid-infrared spectral survey of mass-losing carbon stars in the Large Magellanic Cloud104citations
  • 2005An empirical formula for the mass-loss rates of dust-enshrouded red supergiants and oxygen-rich Asymptotic Giant Branch stars376citations

Places of action

Chart of shared publication
Tafoya, Daniel
1 / 1 shared
Steene, Griet Van De
1 / 2 shared
Hoof, Peter A. M. Van
1 / 1 shared
Barria, Daniela
1 / 1 shared
Randall, Suzanna
1 / 1 shared
Hajduk, Marcin
1 / 1 shared
Unnikrishnan, Ramlal
1 / 1 shared
Toala, Jesus A.
1 / 1 shared
Kimeswenger, Stefan
1 / 1 shared
Mcdonald, Iain
5 / 6 shared
Helton, L. A.
1 / 3 shared
Evans, A.
1 / 14 shared
Worters, H.
1 / 1 shared
Lykou, Foteini
1 / 1 shared
Montiel, E. J.
1 / 2 shared
Starrfield, S.
1 / 3 shared
Banerjee, D. P. K.
1 / 2 shared
Gehrz, R. D.
1 / 5 shared
Richter, M.
1 / 25 shared
Hinkle, K.
1 / 1 shared
Liimets, T.
1 / 1 shared
Woodward, C. E.
1 / 4 shared
Clayton, G. C.
1 / 3 shared
Sarre, P. J.
1 / 1 shared
Eyres, S. P. S.
1 / 2 shared
Krautter, J.
1 / 2 shared
Geballe, T. R.
1 / 5 shared
Joyce, R. R.
1 / 1 shared
Kraemer, Kathleen E.
1 / 2 shared
Keller, Luke D.
1 / 1 shared
Sloan, G. C.
9 / 17 shared
Groenewegen, Martin A. T.
1 / 2 shared
Matsuura, M.
5 / 12 shared
Kemper, F.
2 / 5 shared
Srinivasan, S.
2 / 17 shared
Loon, J. Th. Van
1 / 2 shared
Boyer, M. L.
2 / 2 shared
Wood, P. R.
5 / 9 shared
Kraemer, K. E.
3 / 7 shared
Groenewegen, M. A. T.
6 / 13 shared
Lagadec, E.
4 / 7 shared
Sahai, R.
4 / 5 shared
Volk, K.
2 / 4 shared
Sargeant, B. A.
2 / 2 shared
Th. Van Loon, J.
1 / 1 shared
Tielens, A. G. G. M.
2 / 16 shared
Loon, J. Th Van
4 / 4 shared
Feast, M. W.
4 / 7 shared
Decin, L.
1 / 2 shared
Wyk, F. Van
1 / 1 shared
Smolders, K.
1 / 3 shared
Hony, S.
3 / 7 shared
Gutenkunst, S.
1 / 1 shared
Bernard-Salas, J.
3 / 8 shared
Peeters, E.
1 / 6 shared
Houck, J. R.
2 / 5 shared
Devost, D.
1 / 1 shared
Olivier, E. A.
1 / 2 shared
Cioni, M. R. L.
4 / 7 shared
Blommaert, J. A. D. L.
2 / 4 shared
Vanhollebeke, E.
1 / 2 shared
Menzies, J. W.
3 / 6 shared
Habing, H. J.
2 / 4 shared
Whitelock, P. A.
3 / 6 shared
Harris, G. J.
1 / 2 shared
Loup, C.
2 / 3 shared
Wood, Peter R.
1 / 2 shared
Loon, Jacco Th Van
1 / 1 shared
Waters, L. B. F. M.
1 / 14 shared
Lagadec, Eric
1 / 3 shared
Matsuura, Mikako
1 / 9 shared
Chart of publication period
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2021
2020
2019
2016
2014
2011
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Co-Authors (by relevance)

  • Tafoya, Daniel
  • Steene, Griet Van De
  • Hoof, Peter A. M. Van
  • Barria, Daniela
  • Randall, Suzanna
  • Hajduk, Marcin
  • Unnikrishnan, Ramlal
  • Toala, Jesus A.
  • Kimeswenger, Stefan
  • Mcdonald, Iain
  • Helton, L. A.
  • Evans, A.
  • Worters, H.
  • Lykou, Foteini
  • Montiel, E. J.
  • Starrfield, S.
  • Banerjee, D. P. K.
  • Gehrz, R. D.
  • Richter, M.
  • Hinkle, K.
  • Liimets, T.
  • Woodward, C. E.
  • Clayton, G. C.
  • Sarre, P. J.
  • Eyres, S. P. S.
  • Krautter, J.
  • Geballe, T. R.
  • Joyce, R. R.
  • Kraemer, Kathleen E.
  • Keller, Luke D.
  • Sloan, G. C.
  • Groenewegen, Martin A. T.
  • Matsuura, M.
  • Kemper, F.
  • Srinivasan, S.
  • Loon, J. Th. Van
  • Boyer, M. L.
  • Wood, P. R.
  • Kraemer, K. E.
  • Groenewegen, M. A. T.
  • Lagadec, E.
  • Sahai, R.
  • Volk, K.
  • Sargeant, B. A.
  • Th. Van Loon, J.
  • Tielens, A. G. G. M.
  • Loon, J. Th Van
  • Feast, M. W.
  • Decin, L.
  • Wyk, F. Van
  • Smolders, K.
  • Hony, S.
  • Gutenkunst, S.
  • Bernard-Salas, J.
  • Peeters, E.
  • Houck, J. R.
  • Devost, D.
  • Olivier, E. A.
  • Cioni, M. R. L.
  • Blommaert, J. A. D. L.
  • Vanhollebeke, E.
  • Menzies, J. W.
  • Habing, H. J.
  • Whitelock, P. A.
  • Harris, G. J.
  • Loup, C.
  • Wood, Peter R.
  • Loon, Jacco Th Van
  • Waters, L. B. F. M.
  • Lagadec, Eric
  • Matsuura, Mikako
OrganizationsLocationPeople

article

The Herschel planetary nebula survey (HerPlaNS): I. Data overview and analysis demonstration with NGC? 6781

  • Zijlstra, Albert
  • Rattray, R. E.
  • Exter, K. M.
  • Behar, E.
  • Montez, R.
  • Izumiura, H.
  • Sandin, C.
  • Szczerba, R.
  • Sahai, R.
  • Vlemmings, W.
  • Nordon, R.
  • Otsuka, M.
  • Mcdonald, I.
  • Ladjal, D.
  • Tielens, A. G. G. M.
  • Yamamura, I.
  • Lopez, J. A.
  • Hora, J. L.
  • Chu, Y. H.
  • Kastner, J. H.
  • Hebden, K.
  • Marco, O. De
  • Hoof, P. A. M. Van
  • Wittkowski, M.
  • Ramstedt, S.
  • Balick, B.
  • Villaver, E.
  • Aleman, I.
  • Ueta, T.
  • Nordhaus, J.
  • Blackman, E. G.
  • Murakawa, K.
  • Siódmiak, N.
Abstract

Context. This is the first of a series of investigations into far-IR characteristics of 11 planetary nebulae (PNe) under the Herschel Space Observatory open time? 1 program, Herschel Planetary Nebula Survey (HerPlaNS). Aims. Using the HerPlaNS data set, we look into the PN energetics and variations of the physical conditions within the target nebulae. In the present work, we provide an overview of the survey, data acquisition and processing, and resulting data products. Methods. We performed (1) PACS/SPIRE broadband imaging to determine the spatial distribution of the cold dust component in the target PNe and (2) PACS/SPIRE spectral-energy-distribution and line spectroscopy to determine the spatial distribution of the gas component in the target PNe. Results. For the case of NGC? 6781, the broadband maps confirm the nearly pole-on barrel structure of the amorphous carbon-rich dust shell and the surrounding halo having temperatures of 26-40? K. The PACS/SPIRE multiposition spectra show spatial variations of far-IR lines that reflect the physical stratification of the nebula. We demonstrate that spatially resolved far-IR line diagnostics yield the (Te, ne) profiles, from which distributions of ionized, atomic, and molecular gases can be determined. Direct comparison of the dust and gas column mass maps constrained by the HerPlaNS data allows to construct an empirical gas-to-dust mass ratio map, which shows a range of ratios with the median of 195 ± 110. The present analysis yields estimates of the total mass of the shell to be 0.86? M?, consisting of 0.54? M? of ionized gas, 0.12? M? of atomic gas, 0.2? M? of molecular gas, and 4 × 10-3? M? of dust grains. These estimates also suggest that the central star of about 1.5? M? initial mass is terminating its PN evolution onto the white dwarf cooling track. Conclusions. The HerPlaNS data provide various diagnostics for both the dust and gas components in a spatially resolved manner. In the forthcoming papers of the HerPlaNS series we will explore the HerPlaNS data set fully for the entire sample of 11 PNe. © ESO 2014.

Topics
  • impedance spectroscopy
  • amorphous
  • Carbon
  • grain