It’s not often you get to be in the room with a giant space telescope.

But this time it’s actually happening.

A new paper in the Journal of Geophysical Research Letters says that a team of researchers led by James C. McElroy of the Space Telescope Science Institute has successfully created the first “Star press” that can actually capture and manipulate the gravitational waves produced by a massive star in the center of a galaxy.

The team’s study was based on the new technique that is being developed to capture the light from the massive star.

The Star Press technique would allow astronomers to make observations of the massive stars in the centers of galaxies.

By taking a photo of a distant object, the telescope could then measure the light’s intensity, which could be used to measure the speed of light in the vicinity.

It could also be used for observations of massive stars as well.

In a paper co-authored by McElry, his co-authors, Jie Wang and Jia-Zhi Zhou, describe how the technique can produce high-resolution images of a star that can be “pitched out” to a field of stars in a galaxy with many thousands of stars.

The technique is based on a technique called “light microscopy,” which is similar to the way we can image stars in our field of view by using special light detectors.

“The Star press technique will allow us to see objects in the infrared of a black hole, but in this case we can also see stars in infrared, which would have been previously very difficult to do,” said McElroys co-author of the paper, David C. Hwang.

McElroy is the former chair of the Joint ALMA team, and is now a professor of physics at the University of California, Santa Barbara.

The Star Press method was developed by McAlroy and Wang, and the team is funded by the European Space Agency, NASA and the National Science Foundation.

The technique involves using a specialized light microscope to see a portion of a large galaxy, called a supermassive black hole.

These are massive stars that reside in the centres of galaxies, where the gravity of the galaxies is strong enough to cause them to collapse into one another.

This collapse creates a massive shock wave, which can then be measured.

In the case of a superhot star like our sun, the shock wave would travel at around 1,000 times the speed with which light travels in the universe, which is roughly 10 billion kilometers per second.

This shock wave is emitted by a star, and its light is reflected by a camera.

When the star reaches the camera, the light is absorbed by the lens, which allows the researchers to measure how much of that light is captured by the telescope.

They then can compare that to the light captured by a light microscope, and adjust the light intensity.

For example, if the shockwave intensity is less than 0.5 percent of the intensity of the light coming from the camera in a region where the star is, say, 500 light years away, the researchers can calculate the size of the galaxy that is producing the shockwaves.

In other words, the star could be detected using an instrument that can take the light of the star and magnify it to a few percent of its brightness.

To produce these images, the team’s laser is focused on the tip of a giant laser telescope called the ALMA, which uses a combination of lasers and X-ray beams to detect the light that bounces off of the stars’ supermassive cores.

By measuring the intensity and shape of the optical wave coming off of this supermassive core, they can then use that information to measure light from nearby stars.

The new technique could allow astronomers not only to take high-res images of distant objects, but also to take images of supermassive stars, which are much larger and therefore require much longer exposures.

One thing that is particularly exciting about this work is that it takes advantage of the fact that supermassive systems are made of hydrogen, which has a very low mass, meaning that it has a lot of energy and it’s very difficult for a light detector to capture light from that.

That’s what makes this technique so useful.

“One of the major challenges is the energy density of the hydrogen,” McElron said.

“That heat is then reflected by these supermassive mirrors, which create this huge shockwave. “

So the only way to capture this energy is to take a laser beam that is focused onto the supermassive mirror and then you use the energy from”

That heat is then reflected by these supermassive mirrors, which create this huge shockwave.

So the only way to capture this energy is to take a laser beam that is focused onto the supermassive mirror and then you use the energy from