Stellar motions in outer halo shed new light on Milky Way evolution

Feb 21, 2013
his illustration shows the disk of our Milky Way galaxy, surrounded by a faint, extended halo of old stars. Astronomers using the Hubble Space Telescope to observe the nearby Andromeda galaxy serendipitously identified a dozen foreground stars in the Milky Way halo. They measured the first sideways motions (represented by the arrows) for such distant halo stars. The motions indicate the possible presence of a shell in the halo, which may have formed from the accretion of a dwarf galaxy. This observation supports the view that the Milky Way has undergone continuing growth and evolution over its lifetime by consuming smaller galaxies. Credit: NASA, ESA, and A. Feild (STScI)

(Phys.org)—Peering deep into the vast stellar halo that envelops our Milky Way galaxy, astronomers using NASA's Hubble Space Telescope have uncovered tantalizing evidence for the possible existence of a shell of stars that are a relic of cannibalism by our Milky Way.

Hubble was used to precisely measure, for the first time ever, the sideways motions of a small sample of stars located far from the galaxy's center. Their unusual lateral motion is circumstantial evidence that the stars may be the remnants of a shredded galaxy that was gravitationally ripped apart by the Milky Way billions of years ago. These stars support the idea that the Milky Way grew, in part, through the accretion of smaller galaxies.

"Hubble's unique capabilities are allowing astronomers to uncover clues to the galaxy's remote past. The more distant regions of the galaxy have evolved more slowly than the inner sections. Objects in the outer regions still bear the signatures of events that happened long ago," said Roeland van der Marel of the Space Telescope Science Institute (STScI) in Baltimore, Md.

They also offer a new opportunity for measuring the "hidden" mass of our galaxy, which is in the form of dark matter (an invisible form of matter that does not emit or reflect radiation). In a universe full of 100 billion galaxies, our Milky Way "home" offers the closest and therefore best site for detailed study of the history and architecture of a galaxy.

A team of astronomers led by Alis Deason of the University of California, Santa Cruz, and van der Marel identified 13 stars located roughly 80,000 light-years from the galaxy's center. They lie in the Milky Way's outer halo of that date back to the formation of our galaxy.

The team was surprised to find that the stars showed more of a sideways, or tangential, amount of motion than they expected. This movement is different from what astronomers know about the halo stars near the Sun, which move predominantly in radial orbits. Stars in these orbits plunge toward the galactic center and travel back out again. The stars' tangential motion can be explained if there is an over-density of stars at 80,000 light-years, like cars backing up on an expressway. This traffic jam would form a shell-like feature, as seen around other galaxies.

Deason and her team plucked the outer halo stars out of seven years' worth of archival Hubble telescope observations of our neighboring Andromeda galaxy. In those observations, Hubble peered through the Milky Way's halo to study the Andromeda stars, which are more than 20 times farther away. The Milky Way's halo stars were in the foreground and considered as clutter for the study of Andromeda. But to Deason's study they were pure gold. The observations offered a unique opportunity to look at the motion of Milky Way halo stars.

Finding the stars was meticulous work. Each Hubble image contained more than 100,000 stars. "We had to somehow find those few stars that actually belonged to the Milky Way halo," van der Marel said. "It was like finding needles in a haystack."

The astronomers identified the stars based on their colors, brightnesses, and sideways motions. The halo stars appear to move faster than the Andromeda stars because they are so much closer. Team member Sangmo Tony Sohn of STScI identified the halo stars and measured both the amount and direction of their slight sideways motion. The stars move on the sky only about one milliarcsecond a year, which would be like watching a golf ball on the Moon moving one foot per month. Nonetheless, this was measured with 5 percent precision, made possible in visible-light observations because of Hubble's razor-sharp view and instrument consistency.

"Measurements of this accuracy are enabled by a combination of Hubble's sharp view, the many years' worth of observations, and the telescope's stability. Hubble is located in the space environment, and it's free of gravity, wind, atmosphere, and seismic perturbations," van der Marel said.

Stars in the inner halo have highly radial orbits. When the team compared the tangential motion of the outer halo stars with their radial motion, they were very surprised to find that the two were equal. Computer simulations of galaxy formation normally show an increasing tendency towards radial motion if one moves further out in the halo. These observations imply the opposite trend. The existence of a shell structure in the Milky Way halo is one plausible explanation of the researchers' findings. Such a shell can form by accretion of a satellite galaxy. This is consistent with a picture in which the Milky Way has undergone continuing evolution over its lifetime due to the accretion of satellite galaxies.

The team compared their results with data of halo stars recorded in the Sloan Digital Sky Survey. Those observations uncovered a higher density of stars at about the same distance as the 13 outer halo stars in their Hubble study. A similar excess of halo stars exists across the Triangulum and Andromeda constellations. Beyond that radius, the number of stars plummets.

Deason immediately thought the two results were more than just coincidence. "What may be happening is that the stars are moving quite slowly because they are at the apocenter, the farthest point in their about the hub of our Milky Way," Deason explained. "The slowdown creates a pileup of stars as they loop around in their path and travel back towards the galaxy. So their in and out or radial motion decreases compared with their sideways or tangential motion."

Shells of stars have been seen in the halos of some galaxies, and astronomers predicted that the Milky Way may contain them, too. But until now there was limited evidence for their existence. The halo stars in our galaxy are hard to see because they are dim and spread across the sky.

Encouraged by this study, the team hopes to search for more distant halo stars in the Hubble archive. "These unexpected results fuel our interest in looking for more stars to confirm that this is really happening," Deason said. "At the moment we have quite a small sample. So we really can make it a lot more robust with getting more fields with Hubble." The Andromeda observations only cover a very small "keyhole view" of the sky.

The team's goal is to put together a clearer picture of the Milky Way's formation history. By knowing the orbits and motions of many halo stars it will also be possible to calculate an accurate mass for the galaxy. "Until now, what we have been missing is the stars' tangential motion, which is a key component. The tangential motion will allow us to better measure the total mass distribution of the galaxy, which is dominated by dark matter. By studying the mass distribution, we can see whether it follows the same distribution as predicted in theories of structure formation," Deason said.

The Hubble study will appear in an upcoming issue of the Astrophysical Journal.

Explore further: Violent origins of disc galaxies probed by ALMA

More information: Research paper by A. Deason (University of California, Santa Cruz), et al., accepted for publication in ApJ, 2013 (PDF document): hubblesite.org/pubinfo/pdf/2013/07/pdf.pdf

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cantdrive85
1.4 / 5 (9) Feb 21, 2013
The "shell" is not unexpected in the PC model, the various plasma layers of the Earth's and Sun's EM fields (like layers of an onion) show this is an expected result of plasma interactions. The scalability of EM plasma interactions suggests that the galaxy's EM field will be a larger version of the solar EM field and so on down to the atomic structure.
typicalguy
1 / 5 (5) Feb 21, 2013
I have an idea, let's crash Hubble into the atmosphere and burn it up! The government hates science now anyway and don't want to fund it.
ValeriaT
1 / 5 (4) Feb 21, 2013
This finding is not so surprising. For example, Andromeda galaxy exhibits some shell around its core, which is quite apparent in X-ray spectrum. And the Milky Way galaxy - which is younger but otherwise quite similar to Andromeda - will not be very different. Many findings are quite easy if you know where to look for it - so you should be informed first.
ValeriaT
1 / 5 (4) Feb 21, 2013
The shell in many galaxies represents the shock or bow wave, resulting from less or more apparent activity of their core. I presume, even seemingly quiet galactic centers may ejects less or more steady jets of neutrinos, which do annihilate with CMBR background and interstellar gas around galaxy and which are forming less or more compact halo or sphere of newly created particles there.

Errata: IMO Milky Way is older - not younger - than the Andromeda galaxy, which is rather fresh product of galactic merger in addition.
ValeriaT
1 / 5 (5) Feb 21, 2013
Note that the shell of Andromeda galaxy exhibits dodecahedral structure composed of adjacent voids like the cluster of foam bubbles. It would indicate, that central black holes exhibits whole bundle of neutrino jets or that the dark matter around it exhibits cohesive foam behavior. In my model the activity of central black holes ceases gradually and the active galactic nuclei is losing one its jets one after another.
yyz
4.4 / 5 (7) Feb 21, 2013
"...Andromeda galaxy exhibits some shell around its core, which is quite apparent in X-ray spectrum."

Do you have a link to a published paper describing this X-ray "shell" in M31?

The images you linked to showing a purported X-ray "shell" in M31:

http://1.bp.blogspot.com/_HkkJKGa-ZX8/TSSJE4x4n1I/AAAAAAAAAVc/T5_zW-WCFdI/s1600/Andromeda%20Galaxy%20in%20X-rays.jpg

http://www.aether...hell.gif

reveal nothing more than instrumental artifacts resulting from the (inaccurate) assembly of X-ray mosaics from early XMM-Newton data (i.e. they do not correspond to real XR structures in M31). Compare those images to properly callibrated XR mosaics of M31 from both XMM and Chandra data(see Fig 1):

http://arxiv.org/abs/1002.3353

The shell structure detected in this study is stellar in nature and similar to stellar shells/ripples detected in many galaxies suspected of undergoing a past merger(i.e. http://apod.nasa....226.html ).

yyz
5 / 5 (7) Feb 21, 2013
"...Andromeda galaxy exhibits some shell around its core, which is quite apparent in X-ray spectrum."

To reiterate, this current study discusses a shell of stars discovered some 24kpc from the galactic center of the Milky Way Galaxy and not a fictitious XR shell within a kpc of the nucleus of M31: http://arxiv.org/abs/1302.5111
Anda
5 / 5 (3) Feb 22, 2013
Thank you yyz for your true scientific comments, and sorry for my first (wrong) vote. I thought it was "waterripples" comment (one of many).
Torbjorn_Larsson_OM
5 / 5 (3) Feb 22, 2013
Antiscientists (there is no "PC model" qualifying as science, and so such comments doesn't belong on science sites) and sockpuppetry. WWES - what would Einstein say?