Walk-Only Zones help keep Tempe campus safe

April 29, 2014

Following nearly eight months of campus education about the Walk-Only Zones on ASU's Tempe campus, the university community is now expected to comply to the newly introduced Campus Mall Enforcement program, which took effect March 31.

Watch the video. Campus Mall Enforcement staff on ASU's Tempe campus Download Full Image

Established Aug. 1, 2013, the Walk-Only Zones were aimed at enhancing pedestrian safety by easing vehicle congestion in heavily traveled areas. During enforcement times (8 a.m.-4 p.m., Monday-Friday), no one may ride, drive or park wheeled vehicles in these areas.

ASU students, faculty and staff who do not follow guidelines during zone enforcement times are now subject to a three-tiered enforcement process:

• First violation: A Campus Mall Enforcement staff member issues individuals who are not observing Walk-Only Zones guidelines a written warning.

• Second violation: Students must attend an ASU Police Department Bicycle Safety class. Faculty and staff must attend an ASU Driving on the Mall class.

• Third violation: Individuals will receive a referral to the dean of students, dean or vice president.

Violation notices are posted to individual ASU transportation accounts. Visit parking.asu.edu and navigate to MyParking Online Services. ASU Parking and Transit Services do not oversee Zones enforcement.

It is important to note that the zones are not intended to limit or redirect use of mobility devices by individuals with disabilities.

Tempe campus infrastructure created to support Walk-Only Zones includes bicycle racks in a variety of types and locations, as well as: card-access storage facility, bicycle valet service, daytime-only golf cart parking areas and locked skateboard racks.

Additional details about zone enforcement, including the ASU Transportation Policy and Bicycle Safety class schedules, can be found at: walk.asu.edu/enforcement.html.

Submit Walk-Only Zones questions or comments via the feedback form on walk.asu.edu under the “Contact” tab.

Wendy Craft

Marketing and communications manager, Business and Finance Communications Group


ASU researchers find young galaxies not behaving as expected

April 29, 2014

New Herschel Space Observatory findings have given scientists a remarkable insight into the internal dynamics of two young galaxies. Surprisingly, they have shown that just a few billion years after the big bang, some galaxies were rotating in a mature way, seemingly having completed the accumulation of their gas reservoirs.

When galaxies form, they accumulate mass by gravitationally attracting vast, external gas clouds. As the gas clouds are consumed by the galaxy, they fall into haphazard orbits. These disordered paths cause turbulence in the host galaxies, which can drive star formation. young galaxy Download Full Image

To investigate the internal conditions of forming galaxies, James Rhoads and Sangeeta Malhotra, both from Arizona State University, and colleagues targeted two young galaxies, known as SDSS0901 and the Clone. The light from both galaxies has taken 10 billion years to reach us across space. Thus, we are seeing them when they were comparatively young.

Rhoads studies galaxy formation, galaxy evolution and the reionization of intergalactic hydrogen by early galaxies. Malhotra’s research ranges from properties of dust and gas in the (relatively nearby) interstellar medium to some of the farthest known galaxies. In recent years they have also collaborated on finding and characterizing galaxies in the cosmic dawn, when the universe was less than a billion years old.

The current project focuses on a somewhat later time, the high noon of star formation in the universe – a time when the universe was about 3 billion years old, and when star birth in galaxies was much more active than it is today.

“The purpose of this project is to study the physical conditions of gas in those galaxies. We wanted to know: 'Are they similar to the galaxies around us, or is there some difference in their physical conditions?'” says Rhoads.

The two galaxies they choose to study are average galaxies for that time in cosmic history. This means that they are about 10 to 20 percent the size of our Milky Way, which is considered an average galaxy in the present-day universe.

Studying galaxies so far away is usually challenging because they appear too dim to study effectively, but in this case, the researchers were helped by a cosmic mirage known as a gravitational lens. The two galaxies both sit behind intervening groups of galaxies, whose gravity warps space. As described by Albert Einstein’s General Theory of Relativity, this warping acts like a lens. Although it distorts the images of the young galaxies, it helps by magnifying their light, thus bringing them within reach of Herschel’s HIFI instrument.

The researchers used HIFI to investigate the infrared light of ionized carbon, which is emitted at a wavelength of 158 micrometers. This spectral line is produced in the clouds that surround star-forming regions. HIFI showed the line was broadened into a double peak, and this allowed the motion of the gas to be fitted with a model.

“The two peaks represent two sides of a rotating galaxy. One side is rotating away from us and the other is coming toward us. The broadening of the peaks gives us an indication of the randomness of the motion on top of rotation,” explains Malhotra.

First, the team fitted the overall rotation of the galaxy, and then the turbulence in the gas clouds. To their surprise, they found that galaxy S0901 was extremely well behaved. Instead of turbulence, it was found to be in orderly rotation, much more akin to the majestic galaxies of today.

“Usually, when astronomers examine galaxies at this early era, they find that turbulence plays a much greater role than it does in modern galaxies. But S0901 is a clear exception to that pattern, and the Clone could be another,” says Rhoads.

The Clone, the second galaxy in their study, could also be fitted by an orderly rotation. However, because it was somewhat dimmer, the quality of the data was not so good. This meant that the data could also be fitted with a highly turbulent model, as conventional wisdom would expect.

“Galaxies 10 billion years ago were making stars more actively than they do now,” says Malhotra. "They usually also show more turbulence, likely because they are accumulating gas faster than a modern galaxy does. But here, we have cases of early galaxies that combine the ‘calm’ rotation of a modern one with the active star formation of their early peers. This suggests first that these galaxies have finished accumulating their gas, at least for now. But it also seems that turbulence is not actually required to trigger that early, active star formation."

Malhotra acknowledges the preliminary nature of their study. “This is not the last word on this. We need a bigger sample to be sure of our conclusions,” she says.

But that bigger sample will not be investigated by Herschel. As predicted, the liquid helium coolant needed to keep HIFI and Herschel’s other instruments working ran out in April 2013. Instead, the researchers hope to continue the work pioneered by Herschel using the Atacama Large Millimetre Array (ALMA), a ground-based array of 66 radio dishes in Chile.

“It is mind-boggling that with Herschel/HIFI – admittedly with the help of gravitational lensing – it has been possible to study the internal gas kinematics in galaxies when the universe was only a few billion years old, and what we can learn about them this way. This pioneering work by Herschel is bound to be continued,” says Göran Pilbratt, Herschel Project scientist at the European Space Agency.

Nikki Cassis

marketing and communications director, School of Earth and Space Exploration