Distant Stars Spotted for the First Time in the Vast Magellanic Stream

Artist's rendition of the Magellanic Stellar Stream. The Milky Way's nearest neighboring galaxies - the Small and Large Magellanic Clouds - are shown on the right side of the illustration. As these galaxies move to the right, the gaseous Magellanic Stream billows behind them, intertwining and stretching across the southern sky. The illustration also shows the 13 red giant stars discovered in the Magellanic Stellar Stream. Image Credits: CfA / Melissa Weiss. High Resolution Image / Low Resolution Image

All-sky map of stars observed by the Gaia space observatory in 'galactic' coordinates, looking towards the center of the Milky Way. The neutral hydrogen gas of the Magellanic Stream is displayed in blue, spanning almost the entire southern sky. Red stars indicate the thirteen red giant stars identified by Chandra et al. to be members of the Magellanic Stellar Stream.  Credit: Red giants: CfA/Vedant Chandra/Melissa Weiss. All-sky view: Gaia Data Processing and Analysis Consortium (DPAC); A. Moitinho/A. F. Silva/M. Barros/C. Barata, University of Lisbon, Portugal; H. Savietto, Fork Research, Portugal. Magellanic Stream data: D. Nidever et al., NRAO/AUI/NSF, Leiden-Argentine-Bonn Survey; Parkes, Westerbork, and Arecibo Observatories. High Resolution Image / Low Resolution Image

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Astronomers have solved a half-century-old scientific mystery by identifying stars associated with the cosmic gas stream emanating from a pair of nearby galaxies.

Cambridge, Mass. – For nearly fifty years, astronomers have come up empty-handed in their search for stars within the sprawling structure known as the Magellanic Stream. A colossal ribbon of gas, the Magellanic Stream spans nearly 300 Moon diameters across the Southern Hemisphere’s sky, trailing behind the Magellanic Cloud galaxies, two of our Milky Way Galaxy’s closest cosmic neighbors.

Now the star search is finally over. Researchers at the Center for Astrophysics | Harvard & Smithsonian (CfA) and colleagues have identified 13 stars whose distances, motion, and chemical makeup place the stars squarely within the enigmatic stream.

Locating these stars has now pinned down the true distance to the Magellanic Stream, revealing that it extends from 150,000 light-years to more than 400,000 light-years away. The findings pave the way to map and model the Magellanic Stream in unprecedented detail, offering new insights into the history and characteristics of our Galaxy and its neighbors.

"The Magellanic Stream dominates the Southern Hemisphere's sky and our work has at last found a stellar structure that people have sought for decades," says Vedant Chandra, a PhD student in Astronomy & Astrophysics at the CfA and lead author of a new study published in The Astrophysical Journal reporting the findings.

"With these results and more like them, we hope to gain a far greater understanding of the formation of the Magellanic Stream and the Magellanic Clouds, as well as their past and future interactions with our Galaxy," said co-author Charlie Conroy, a Professor of Astronomy at the CfA and Chandra’s advisor.

The Large and Small Magellanic Clouds are dwarf satellite galaxies of the Milky Way. Visible to the naked eye as gauzy luminances, the Clouds have been known since antiquity. With the advent of increasingly powerful telescopes able to perceive phenomena too faint for our eyes to see, astronomers discovered a gigantic plume of hydrogen gas apparently cast out of the Clouds in the early 1970s.

Studies of the gas within this Magellanic Stream further showed the Stream to have two interwoven filaments, with one originating from each Cloud. These features suggest the gravity of the Milky Way might have pulled the Magellanic Stream out of the Clouds. Yet how exactly the Stream formed has remained difficult to nail down, in no small part because of its presumed stellar component remaining irksomely indiscernible.

Chandra came at this problem through an ambitious project started in 2021 for his PhD at the CfA. Chandra consulted with Conroy about interesting topic areas to study, and Conroy pointed Chandra to the uncharted frontier of the Milky Way. The scant stars dotting the Galaxy’s outskirts have been little studied because our Solar System is smack dab in the starry disk of the Milky Way itself—akin to a concertgoer near the stage attempting to see somebody all the way out at the crowd’s periphery.

Over the last decade though, deep observational catalogs compiled by new instruments—especially the European Space Agency's Gaia spacecraft—have started to spy stellar objects that just might be these elusive frontier stars. With access granted to the 6.5m Magellan Baade Telescope at Las Campanas Observatory in Chile through the CfA and MIT, Chandra undertook a project to perform spectroscopy on 200 far-flung Milky Way stars, which when completed will be the largest such sample set to date.

Spectroscopy involves collecting enough light from an object to detect certain signatures imprinted within the light’s color bands that, like fingerprints, uniquely identify individual chemical elements. These signatures thus disclose the chemical makeup of an object, speaking to its origins. In addition, the signatures shift based on the distance to an object, enabling astronomers to tell where an object, such as a star, is going, and correspondingly where it came from.

In the case of Chandra's study, the spectroscopic analysis revealed a set of 13 stars with distances and velocities that fall right within the range expected for the Magellanic Stream. What’s more, the stars’ chemical abundances matched those of the Magellanic Clouds, for instance by being distinctively deficient in the heavier elements astronomers call metals. “These 13 stars just fell right out of our dataset,” says Rohan Naidu, co-author on the study and former CfA graduate student, currently a Hubble postdoctoral fellow at MIT.

By obtaining solid distance and extent measurements of the Magellanic Stream via these stars, the researchers buttressed its origin story as a gravitational grab by the Milky Way. The researchers were additionally able to calculate the Stream's overall gas distribution with higher confidence compared to prior estimates. The distribution indicates that the Stream is actually about twice as massive as generally reckoned.

That result, in turn, presages a future full of new star formation in the Milky Way, because the Stream is actively falling into our Galaxy, according to previous observations. In this way, the Stream serves as a primary provider of the cold, neutral gas needed for making fresh Milky Way stars.

"The Magellanic Stream is the dominant source of stellar calories for the Milky Way—it's our breakfast, lunch, and dinner," says Ana Bonaca, co-author on the study and former ITC postdoctoral fellow at the CfA, now staff scientist at Carnegie Observatories. "Based on the new, higher mass estimates for Magellanic Stream, the Milky Way may end up packing on more pounds than initially thought."

Further studies of the Magellanic Stream should also help astronomers learn more about the composition of our Galaxy. Because the Stream is thought to trace the past paths of the Magellanic Clouds, modeling the evolution of the relatively massive Large Magellanic Cloud via the Stream will improve measurements of the Milky Way’s mass distribution. Much of that mass is in the form of dark matter—a poorly understood, gravity-exerting substance. Better gauging the mass of our Galaxy out in its distant hinterlands will aid in accounting for ordinary matter versus dark matter contents, constraining the possible properties of the latter.

"The beauty of having a vast stellar stream like the Magellanic Stream is that we can now perform so many astrophysical investigations with it," says Chandra. "As our spectroscopic survey continues and we find more stars, we're excited to see what other surprises the Galactic outskirts have in store for us."

Source: Harvard-Smithsonian Center for Astrophysics (CfA)/News

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Giant Intergalactic Gas Stream Longer than Thought

Combined radio/optical image shows Milky Way, Magellanic Clouds, and the new radio image of the Magellanic Stream. Blue and white are the Milky Way and Magellanic Clouds. Red is the hydrogen gas in the Magellanic Stream, in the disks of the Magellanic Clouds, and in the stream's Leading Arm. The Milky Way is horizontal in the middle of the image; the Magellanic Clouds are the light spots at the center-right portion of the image, from which the gas stream originates. Brown is dust clouds in the Milky Way. CREDIT: Nidever, et al., NRAO/AUI/NSF and Meilinger, Leiden-Argentine-Bonn Survey, Parkes Observatory, Westerbork Observatory, Arecibo Observatory. Large image with labels

The astronomers used the National Science Foundation's Robert C. Byrd Green Bank Telescope (GBT) to fill important gaps in the picture of gas streaming outward from the Magellanic Clouds. The first evidence of such a flow, named the Magellanic Stream, was discovered more than 30 years ago, and subsequent observations added tantalizing suggestions that there was more. However, the earlier picture showed gaps that left unanswered whether this other gas was part of the same system.

"We now have answered that question. The stream is continuous," said David Nidever, of the University of Virginia. "We now have a much more complete map of the Magellanic Stream," he added. The astronomers presented their findings to the American Astronomical Society's meeting in Washington, DC.

The Magellanic Clouds are the Milky Way's two nearest neighbor galaxies, about 150,000 to 200,000 light-years distant from the Milky Way. Visible in the Southern Hemisphere, they are much smaller than our Galaxy and may have been distorted by its gravity.

Nidever and his colleagues observed the Magellanic Stream for more than 100 hours with the GBT. They then combined their GBT data with that from earlier studies with other radio telescopes, including the Arecibo telescope in Puerto Rico, the Parkes telescope in Australia, and the Westerbork telescope in the Netherlands. The result shows that the stream is more than 40 percent longer than previously known with certainty.

One consequence of the added length of the gas stream is that it must be older, the astronomers say. They now estimate the age of the stream at 2.5 billion years.

The revised size and age of the Magellanic Stream also provides a new potential explanation for how the flow got started.

"The new age of the stream puts its beginning at about the time when the two Magellanic Clouds may have passed close to each other, triggering massive bursts of star formation," Nidever explained. "The strong stellar winds and supernova explosions from that burst of star formation could have blown out the gas and started it flowing toward the Milky Way," he said.

"This fits nicely with some of our earlier work that showed evidence for just such blowouts in the Magellanic Clouds," said Steven Majewski, of the University of Virginia.

Earlier explanations for the stream's cause required the Magellanic Clouds to pass much closer to the Milky Way, but recent orbital simulations have cast doubt on such mechanisms.

Nidever and Majewski worked with Butler Burton of the Leiden Observatory and the National Radio Astronomy Observatory, and Lou Nigra of the University of Wisconsin. In addition to presenting the results to the American Astronomical Society, the scientists have submitted a paper to the Astrophysical Journal.

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