In November, astronomers at the Max Planck Institute for Extraterrestrial Physics presented new observations of the gas cloud G2 in the galactic centre originally discovered in 2011. These data are in remarkably good agreement with an on-going tidal disruption.
As a complete surprise came the discovery that the orbit of G2 matches that of another gas cloud detected a decade ago, suggesting that G2 might actually be part of a much more extensive gas streamer. This would also match some of the proposed scenarios that try to explain the presence of G2. One such model is that G2 is originating from the wind from a massive star.
April 2014: High-resolution image of the gas cloud G2 at the centre of our Milky Way with the SINFONI instrument at the VLT. The red part of the cloud approaches the 4 million solar masses black hole (indicated with a cross) at velocities of a few thousand km/s. The blue part has already passed the closest distance to the black hole and moves away again. The initially spherical could has been stretched by the strong gravitational field of the black hole by a factor 50 in the direction of motion. The cloud's size from red to blue now corresponds to 900 times the Earth-Sun distance. The solid line shows the orbit of the gas cloud. The dashed lines show the orbit of the star with the best known orbit (S2). The positions of the neighbouring stars are indicated as well.
High-resolution images of the centre of our Milky Way with the SINFONI instrument at the VLT. The two gasclouds G1 and G2 are coloured blue and red, respectively. The dashed lines show the orbits of the star with the best known orbit (S2) as well as the best-fit common orbit for the two gas clouds. The cross marks the position of the 4 million solar mass black hole at the galactic centre.
The gas cloud G2 was originally detected by Stefan Gillessen and his colleagues at the Max Planck Institute for Extraterrestrial Physics (MPE) in 2011. It is on a highly eccentric orbit around the galactic centre and observations in 2013 have shown that part of the gas cloud is already past its closest approach to the black hole, at a distance of roughly 20 light hours (a bit more than 20 billion kilometres or 2000 Schwarzschild radii).
The new, deep infrared observations with the SINFONI instrument at the VLT track the ongoing tidal disruption of the gas cloud by the powerful gravitational field. While the shape and path of the gas cloud agrees well with predictions from the models, so far there has been no significant enhanced high-energy emission, as one might have expected from the associated shock front.
But a closer look into the data set led to a surprise. “Already a decade ago, another gas cloud – which we now call G1 – has been observed in the central region of our galaxy,” remarks Stefan Gillessen. “We explored the connection between G1 and G2 and find an astonishing similarity in both orbits.”
The faint and blurry object G1 can be seen in the data sets from 2004 to 2008. The MPE team was able to determine also G1’s orbit. This revealed that it has already passed pericenter in 2001. The similarity of the orbits thus suggests that G1 is about 13 years ahead of G2. The scientists fed this information into a model for a combined orbit, taking into account the different pericentre times and allowing for slightly different orbits due to interaction of the gas with the ambient medium after pericentre passage.
“Our basic idea is that G1 and G2 might be clumps of the same gas streamer”, explains Oliver Pfuhl, lead author of the study presented in the recent paper. “In this case, we should be able to simultaneously fit both data sets and, indeed, our model captures the G1 and G2 orbits remarkably well.”
The model makes the simple assumption that G1 was decelerated during pericentre passage by a drag force due to the thin atmosphere that surrounds the massive black hole. This drag pushed it into a more circular orbit. Using just this very simple assumption the emission of both G1 and G2 apparently trace the same orbit. Small deviations from the fit are not surprising given the simplicity of the model, which likely is neglecting some essential physics.
“The good agreement of the model with the data renders the idea that G1 and G2 are part of the same gas streamer highly plausible,” states Gillessen. A likely source for both G1 and G2 could then be clumps in the wind of one of the massive disk stars, which could have been ejected some 100 years ago close to the apocentre of the G2 orbit. Another possible explanation that has been suggested recently would be a large star, enveloped by an extended gas cloud. Based on the current VLT data, however, this model is highly unlikely.
Moreover, the gas streamer picture could also help to explain the missing X-ray emission from the gas cloud near the black hole, although the non-detection of such emission is not yet understood.
Phone: +49 (0)89 30000-3852
Fax: +49 (0)89 30000-3569
Phone:+49 (0)89 30000-3839
Fax: +49 (0)89 30000-3390
Phone: +49 (0)89 30000-3980
Fax: +49 (0)89 30000-3569
Oliver Pfuhl, Stefan Gillessen et al.
The Galactic Center cloud G2 and its gas streamer
Accepted for publication in ApJ
Dr. Hannelore Hämmerle | Max-Planck-Institut
Gamma rays will reach beyond the limits of light
23.10.2017 | Chalmers University of Technology
Creation of coherent states in molecules by incoherent electrons
23.10.2017 | Tata Institute of Fundamental Research
Salmonellae are dangerous pathogens that enter the body via contaminated food and can cause severe infections. But these bacteria are also known to target...
University of Maryland researchers contribute to historic detection of gravitational waves and light created by event
On August 17, 2017, at 12:41:04 UTC, scientists made the first direct observation of a merger between two neutron stars--the dense, collapsed cores that remain...
Seven new papers describe the first-ever detection of light from a gravitational wave source. The event, caused by two neutron stars colliding and merging together, was dubbed GW170817 because it sent ripples through space-time that reached Earth on 2017 August 17. Around the world, hundreds of excited astronomers mobilized quickly and were able to observe the event using numerous telescopes, providing a wealth of new data.
Previous detections of gravitational waves have all involved the merger of two black holes, a feat that won the 2017 Nobel Prize in Physics earlier this month....
Material defects in end products can quickly result in failures in many areas of industry, and have a massive impact on the safe use of their products. This is why, in the field of quality assurance, intelligent, nondestructive sensor systems play a key role. They allow testing components and parts in a rapid and cost-efficient manner without destroying the actual product or changing its surface. Experts from the Fraunhofer IZFP in Saarbrücken will be presenting two exhibits at the Blechexpo in Stuttgart from 7–10 November 2017 that allow fast, reliable, and automated characterization of materials and detection of defects (Hall 5, Booth 5306).
When quality testing uses time-consuming destructive test methods, it can result in enormous costs due to damaging or destroying the products. And given that...
Using a new cooling technique MPQ scientists succeed at observing collisions in a dense beam of cold and slow dipolar molecules.
How do chemical reactions proceed at extremely low temperatures? The answer requires the investigation of molecular samples that are cold, dense, and slow at...
23.10.2017 | Event News
17.10.2017 | Event News
10.10.2017 | Event News
23.10.2017 | Life Sciences
23.10.2017 | Physics and Astronomy
23.10.2017 | Health and Medicine