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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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
Summer project: The mysterious hydrogen in the barred spiral galaxy NGC 1672

© N/A

NGC 1672 is a barred spiral galaxy located in a relatively isolated environment, with only four smaller satellites in the MeerKAT field of view, and with regular star forming activity for its mass. Despite this, the MHONGOOSE Survey reveals asymmetries and tail-like structures in the low-column density HI of both NGC 1672 and its satellites (left panel). Such features are typically associated with galaxies in denser, strongly interacting environments. Given the low density of the surrounding intergalactic medium, these structures are likely not caused by ram-pressure stripping alone, but rather by tidal interactions and close flybys. In support of this, all satellites show morphological asymmetries (in both stellar and HI emission) as well as dynamical irregularities.

A 3D tilted-ring model of the HI in NGC 1672 was fitted using 3DBarolo (Di Teodoro & Fraternali 2015), revealing a dual-plateau rotation curve with a rapid rise in rotational velocity at a radius of ~20 kpc (upper right panel). The expected rotational velocity from the baryonic Tully–Fisher relation (Lelli, McGaugh, & Schombert 2015) is consistent with the higher outer-disk velocity, suggesting that this represents the true rotational velocity of the galaxy. The dual plateau points to two possible scenarios: either the presence of two rotating discs, or the bar having a large effect on the motion in the inner regions of the galaxy.

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