Astronomers map new emission line to trace most common molecule in the Universe
Molecular hydrogen (H2) makes up 99% of the cold dense gas in galaxies. So mapping where stars are born basically means measuring H2, which lacks a strong characteristic signature at low temperatures. Astronomers from SRON Netherlands Institute for Space Research and the University of Groningen have now mapped an emission signal from the trace molecule hydrogen fluoride (HF), in a place where the standard trace molecule carbon monoxide is absent. They are the first to produce a map of HF for a region in space, creating a new tool to indirectly map H2. Publication in Astronomy & Astrophysics.
![Astronomers new emissionline](/about-ug/latest-news/news/archief2019/image/1109-astronomen-nieuwe-emissielijn-in-kaart.jpg)
All across galaxies in our Universe, stars are dying and forming. And while our life on Earth is based on a rich jumble of various elements and molecules, the cold dense gas out of which stars form is pretty monotonous with 99% molecular hydrogen (H2). So if you want to map where stars are born, you'd better have a good grasp on how to detect H2. Unfortunately, this material is hard to observe due to a lack of a strong characteristic signal at low temperatures—unlike its atomic cousin (H) which emits radio waves at an easily distinguishable wavelength of 21 cm. Astronomers from SRON Netherlands Institute for Space Research and the University of Groningen have now discovered a new tool to indirectly measure H2, by mapping hydrogen fluoride (HF) and linking its abundance to that of H2.
Hydrogen fluoride
The new tool comes in handy when other tools fail, for example in the Orion Bar, in between regions around the Orion Trapezium stars and the Orion Molecular Cloud. In these areas carbon is ionized, meaning that carbon monoxide (CO)—usually a reliable trace molecule to find H2—can't work as a tracer in this case. Floris van der Tak (SRON/RuG) and his team were surprised to find a characteristic HF signal in data from the Herschel telescope coming from the Orion Bar, as astronomers have previously only detected hydrogen fluoride as a silhouette: HF absorbing other radiation. HF and H2 abundance can be linked because HF is produced in a chemical reaction where H2 reacts with atomic fluorine (F) to form HF and atomic hydrogen (H). Without H2 there is no HF.
Collisions
The team, led by SRON PhD student Ümit Kavak, used their map of HF to examine a few mechanisms through which it could emit its signal. Collisions of HF molecules with electrons and molecular hydrogen turns out to be the main mechanism. The collisions excite the HF molecules to a higher energy state, after which they drop to their ground state while emitting infrared light at a characteristic wavelength of 1.2 THz.
Last modified: | 30 April 2020 4.00 p.m. |
More news
-
17 July 2024
Veni-grants for ten researchers in Groningen
The Dutch Research Council (NWO) has awarded a Veni grant of up to €320,000 each to ten researchers of the University of Groningen and the UMCG. The Veni grants are designed for outstanding researchers who have recently gained a PhD.
-
15 July 2024
Funding for RUG researchers from National Growth Fund programme Circular Plastics NL
For research on making plastics circular, Professors Patrizio Raffa and Katja Loos together receive about 1.2 million euros from the National Growth Fund programme Circular Plastics NL.
-
09 July 2024
NWO Open Technology funding for improving quality 3D printing technology
Dr. Liangliang Cheng receives a NWO OPT grant of EUR 950,000 for research on safer application of metals in 3D printing technology.