Telescopes

ASTRON is responsible for the operations of the Westerbork Synthesis Radio Telescope (WSRT) and the Low Frequency Array (LOFAR).

Astronomy

The astronomical research at ASTRON is closely aligned with the strengths of our facilities LOFAR and WSRT-APERTIF.

Research and Innovation


Radio astronomy delivers important breakthrough technology for our society.

News & Events


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Making discoveries
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ASTRON is the Netherlands Institute for Radio Astronomy, and is part of the Institutes organisation of NWO.
STORIES
Simultaneous optical and radio observations of Perseids

From today (August 11th) up until Friday the yearly Perseids meteor shower will have its peak. This phenomenon is not only interesting for amateur astronomers, professional astronomers will be observing them as well.

Humans of ASTRON: Jorrit Siebenga

In Humans of ASTRON we share stories about the people at ASTRON. Who are the people behind the discoveries and innovations and also, who are the people that make sure that everything runs smoothly? In this second part of the series, we’ll be sharing the story of Jorrit Siebenga, who joined ASTRON in 2017 as research instrument maker.

Women Astronomers Day

Throughout the history of astronomy, women have played essential roles towards astronomical breakthroughs. In this article we highlight but a few of these women identified in history from 1600 to the modern era.

Humans of ASTRON: Emanuela Orrù

In Humans of ASTRON we share stories about the people at ASTRON. Who are the people behind the discoveries and innovations and also, who are the people that make sure that everything runs smoothly? In this second part of the series, we’ll be sharing the story of Emanuela Orrù, support scientist at ASTRON since 2012.

What we look forward to in LOFAR 2.0: Live warning system to study solar eruptions
What we look forward to in LOFAR 2.0: Habitability of alien worlds
What we look forward to in LOFAR 2.0: Cranking up LOFAR’s robustness
What we look forward to in LOFAR 2.0: LOFAR expands to Italy
Nearest fast radio burst source is regularly active
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DAILY IMAGE
Colloquium by Manuel Güdel: A fresh look at the environment of DG Tau

© Manuel Güdel

DG Tau is a single, nearby Young Stellar Object young enough to combine features common to embedded protostars and more evolved, optically revealed classical T Tauri stars. This transition object is therefore a key target to understand stellar accretion and ejection processes. It features a Keplerian disk with a hot, water-rich and strongly variable inner region, relics of a non-Keplerian envelope, accretion streamers, and most prominently a system of co-axial molecular, atomic, and ionized disk winds over a wide range of temperatures and velocities. The most extreme winds form a high-velocity bipolar jet system detected almost down to the disk surface at radio, infrared, optical, UV and surprisingly even X-ray wavelengths.

New JWST/MIRI observations reveal molecular lines of hot water and CO associated with the innermost protoplanetary disk; also, despite DG Tau’s youth, a substantial fraction of dust has grown to micron size. The jet system shows very strong infrared forbidden lines for which I will propose a direct link to the ~4 MK X-ray emitting plasma jet via shock heating and cooling. If successful, such a model will reveal more about the inner workings of the jet.

I will discuss shock models that involve collisional ionization and photoionization, shock self-radiation, recombination and charge exchange that are necessarily evolving away from collisional ionization equilibrium and therefore need to be evolved iteratively in time; I will address some diagnostic power of these models.

EVENTS
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