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Centre for Star and Planet Formation | starplan.dk

Centre for Star and Planet Formation. Our goal is to provide observational and theoretical constraints that will help unravel the early history of our solar system in the context of its astrophysical setting, from collapse of the molecular cloud through condensation and evolution of primitive solids and, ultimately. Searching for presolar clues The planets in our solar system are made up of elements produced in earlier generation of stars. Variation in the isotopic abundance of some of these elements...

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Centre for Star and Planet Formation | starplan.dk | starplan.dk Reviews

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Centre for Star and Planet Formation. Our goal is to provide observational and theoretical constraints that will help unravel the early history of our solar system in the context of its astrophysical setting, from collapse of the molecular cloud through condensation and evolution of primitive solids and, ultimately. Searching for presolar clues The planets in our solar system are made up of elements produced in earlier generation of stars. Variation in the isotopic abundance of some of these elements...

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Centre for Star and Planet Formation | starplan.dk | starplan.dk Reviews

https://starplan.dk

Centre for Star and Planet Formation. Our goal is to provide observational and theoretical constraints that will help unravel the early history of our solar system in the context of its astrophysical setting, from collapse of the molecular cloud through condensation and evolution of primitive solids and, ultimately. Searching for presolar clues The planets in our solar system are made up of elements produced in earlier generation of stars. Variation in the isotopic abundance of some of these elements...

INTERNAL PAGES

starplan.dk

1

The Earth was built from small glass beads | starplan.dk

http://starplan.dk/node/1096

The Earth was built from small glass beads. A new study from an international team that includes scientists from the Centre for Star and Planet Formation suggests that clumps of small glassy particules may be responsible for the formation of giant asteroids and the planetary embryos that collided to form rocky planets like Earth. After the sun was born, the rest of the solar system emerged from a giant rotating cloud of gas and dust known as the protoplanetary disk. The researchers found that, as cho...

2

New State-of-the-art Mass Spectrometer Laboratories | starplan.dk

http://starplan.dk/news/new-state-art-mass-spectrometer-laboratories

New State-of-the-art Mass Spectrometer Laboratories. With thanks to Thermo-Fischer engineers Andy Davis and Ian Winstanley, the two instruments, dubbed. Continued success with European Research Council grants. The prestigious European Research Council grants are awarded as Starting Grants, Consolidator. The Earth was built from small glass beads. A new study from an international team that includes scientists from the Centre for Star and Planet. 75 million CPU hours.

3

All Publications | starplan.dk

http://starplan.dk/publications/year

Chen, C.-H.R. Klessen, R.S. Bernard, J.-P. Lee, M.-Y. Madden, S.C. Star formation rates from young-star counts and the structure of the ISM across the NGC 346/N66 complex in the SMC. Monthly Notices of the Royal Astronomical Society, 448. Van der Wiel, M.H.D. Spatial variation of the cooling lines in the reflection nebula NGC 7023. Astronomy and Astrophysics, 574. Matthews, B.C. Gutermuth, R.A. Huard, T.L. Tothill, N.F.H. Bourke, T.L. Di Francesco, J. Jørgensen, J.K. Allen, L.E. Chapman, N.J. Stellar act...

4

Labs | starplan.dk

http://starplan.dk/labs

Isotope facilities at the Centre for Star and Planet Formation. The Geological Museum within the Natural History Museum of Denmark houses isotope facilities that were first opened March 1, 2009 and expanded in 2011. A clean laboratory purifies elements of interest for analyses by either Thermal Ionization Mass Spectrometery or Multi-Collector Inductively-Coupled Plasma Mass Spectrometry. Four designed in house and built locally), two exhausted hoods and a HEPA-filtered weighing room. Image above: Special...

5

Upcoming Seminars | starplan.dk

http://starplan.dk/seminars

09 Jun 2016 - 13:30. Hot water and methanol: a high-energy interstellar cocktail brewed up in low-mass protostars. Niels Bohr Institute and StarPlan. Deeply embedded low-mass protostars are energetic little beasts. Through winds and jets they drive shocks and outflows. 08 Jun 2016 - 14:00. Transiting Planets in Campaigns 5 and 6 and Asteroseismology of Kepler's Brightest Stars. University of Oxford, UK. 31 May 2016 - 14:00. On the orbital motion of Broad-Line Region clouds. Golestan University, Iran.

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bjerkeli.se

Home

http://bjerkeli.se/index.html

Master of Science Thesis. I am an astronomer, currently working as a postdoctoral researcher in the. Center for Star and Planet Formation. Starplan), Copenhagen, Denmark. My research interests are mainly in the field of star- and planet formation, with focus on the physics and chemistry of molecular outflows and shocks. Before taking up my position at Copenhagen university, I worked as a project assistant at the. Chalmers University of Technology. Sergels väg 9 B. Home: 46 31 208844. Work: 46 31 7538844.

labastro.eu

5. Stellar and planetary formation - Laboratory Astrophysics

http://www.labastro.eu/5.-stellar-and-planetary-formation.html

5 Stellar and planetary formation - Laboratory Astrophysics. 1 Gas phase astrochemistry. 2 Spectroscopy of the ISM. 3 Spectroscopy in hot bodies. 4 Solid state/interstellar ice processes. 5 Stellar and planetary formation. 6 Primitive and planetary material. 7 High energy processes and space plasma. 8 Stellar evolution and nuclear astrophysics. 9 Astrophysical conditions for the emergence of life. Laboratory Astrophysics outside Europe. 5 Stellar and planetary formation. Back to main menu.

matthijs.vanderwiel.org

Matthijs van der Wiel (ASTRON)

http://matthijs.vanderwiel.org/cv.php

Matthijs van der Wiel. Full cv available on request. Education and employment history. Jul 2016 – present. LOFAR support scientist at ASTRON Netherlands Institute for Radio Astronomy. Aug 2014 – Jun. 2016. Postdoc at Niels Bohr Institute. And Centre for Star and Planet Formation. University of Copenhagen (Denmark). Jul 2011 – Jul. 2014. Postdoc at Institute for Space Imaging Science. University of Lethbridge ( AB. Apr 2007 – May 2011. PhD in mathematics and natural sciences, Kapteyn Institute.

labastro.eu

6. Primitive and planetary material - Laboratory Astrophysics

http://www.labastro.eu/6.-primitive-and-planetary-material.html

6 Primitive and planetary material - Laboratory Astrophysics. 1 Gas phase astrochemistry. 2 Spectroscopy of the ISM. 3 Spectroscopy in hot bodies. 4 Solid state/interstellar ice processes. 5 Stellar and planetary formation. 6 Primitive and planetary material. 7 High energy processes and space plasma. 8 Stellar evolution and nuclear astrophysics. 9 Astrophysical conditions for the emergence of life. Laboratory Astrophysics outside Europe. 6 Primitive and planetary material. Nobel gas mass spectrometry /.

kromepackage.org

KROME bootcamp!

http://www.kromepackage.org/bootcamp/2014

September 17 - 19, 2014 GOETTINGEN.

kromepackage.org

KROME package

http://www.kromepackage.org/index.php

Better science through chemistry). KROME is a nice and friendly chemistry package for a wide range of astrophysical simulations. Given a chemical network (in CSV format) it automatically generates all the routines needed to solve the kinetic of the system, modelled as a system of coupled Ordinary Differential Equations. It provides different options which make it unique and very flexible. Any suggestions and comments are welcomed. Please use the krome's users mailing list. Read the Wiki to get started.

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Centre for Star and Planet Formation | starplan.dk

Centre for Star and Planet Formation. Our goal is to provide observational and theoretical constraints that will help unravel the early history of our solar system in the context of its astrophysical setting, from collapse of the molecular cloud through condensation and evolution of primitive solids and, ultimately. Searching for presolar clues The planets in our solar system are made up of elements produced in earlier generation of stars. Variation in the isotopic abundance of some of these elements...

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