2023年6月2日 · The dark feature in the continuum MeerKAT and GBT images is anticorrelated with the Sgr E CO cloud. This dark feature shows similar appearance to many GC molecular clouds that have been identified as radio dark clouds (Yusef-Zadeh 2012).

The Sgr E region, seen in Figure 1, is a star-forming complex located just outside the CMZ, spanning Galactic longitudes from l≈359°.3 –358°.3. The placement of the Sgr E complex in both position and line-of-sight velocity is consistent with the intersec-tion point between the dust lanes and the CMZ, as seen in Figure 2.

2023年6月6日 · Finally, it's also possible that the gravitational potential of our galaxy's central bar is tugging the Sgr E cloud. That could play a role in forming those filaments. A schematic diagram of the...

1993年9月30日 · High-resolution radio continuum and radio recombination line observations of Sgr E, one of the least studied H ii complexes in the Galactic center region, show that the distribution of the...

2022年11月2日 · We report on the discovery of linear filaments observed in the CO (1-0) emission for a ∼2′ field of view toward the Sgr E star-forming region, centered at ( l , b ) = (358.°720, 0.°011). The...

Using almost daily observations since 2006, this program has provided a unique baseline to study the long-term X-ray behavior of the central super-massive black hole Sgr A*. We post daily updates of the Swift data to allow for a quick response if the activity of Sgr A* changes, e.g., due to its interaction with the gas cloud "G2".

2023年6月3日 · On a smaller scale, the prominent Sgr E H II complex G358.7-0.0 provides a vivid example of the nearly radial distribution of short filaments. The bimodal PA distribution suggests a different origin for two distinct filament populations. We argue that the alignment of the short-

2023年6月2日 · We have examined the distribution of the position angle (PA) of the Galactic center filaments with lengths L > 66″ and <66″ as well as their length distribution as a function of PA. We find bimodal...

The group of compact sources in the direction of the Galactic Centre (l=358°.7, b=0°) known as Sgr E has been observed with the Molonglo Observatory Synthesis Telescope at 843 MHz and with the Very Large Array at 1.45 and 4.86 GHz.

This observation of the distant molecular cloud Sgr E, with XMM'slarge effective area, is required to probe putative old outbursts fromSgr A*. It will allow us to complete our global study of the Galacticcenter X-ray diffuse emission, which concludes that multiple shortevents happening few hundred years ago are currently propagating throughthe ...