After decades of patient sleuthing, astronomers have pretty well figured out how stars like the Sun form: within swirling pancakes of gas and dust. The gas in these so-called accretion disks bulks up the growing star, astronomers agree, while jets streaming away in opposing directions carry off angular momentum — negating the "centrifugal force" that otherwise would prevent the swirling gases from spiraling onto the growing star-to-be. The tale is backed up by evidence ranging from Hubble Space Telescope pictures of disk-girdled glows to the fact that our solar system's planets follow coplanar orbits.
But the birth processes of heavy stars — those with at least 8 times our Sun's mass — remain mysterious. After all, those stars are far rarer than lightweight ones, making them hard to study, and they evolve much more rapidly, so it's hard to catch one on the act. What's more, theorists have worried that intense light from a massive protostar might push all accreting matter away, nipping its own growth in the bud. Because of this, some have postulated that big stars form not by accretion but when small stars merge.
However, astronomers using the Submillimeter Array, a recently completed octet of dishes atop Mauna Kea, have garnered strong evidence that accretion can make big stars as well as small ones. The best example yet, some say, appears in today's issue of the weekly science journal Nature. There, Nimesh A. Patel, Salvador Curiel, T. K. Sridharan (Harvard-Smithsonian Center for Astrophysics), and seven colleagues show that Cepheus A HW2, a protostar that packs some 15 solar masses, is surrounded by an elongated, rotating, dust-laden gas cloud — itself likely outweighing our Sun several times over.
Earlier observations by the Very Large Array of radio dishes already had shown jets of plasma squirting in opposing directions from Cepheus A HW2, which is hidden from view at visual wavelengths by interstellar dust. The rotating gas cloud (which is plausibly a disk) and the jets (which are perpendicular to the cloud) "are just the ingredients that would, according to recent theories of accretion, allow the formation of massive stars," writes Barbara A. Whitney (Space Science Institute), a star-formation expert who is not a member of Patel's team.
Not that Cepheus A HW2 is the only example of a massive, B-type star being birthed within a disk of some sort, says Debra Shepherd (National Radio Astronomy Observatory). In fact, Shepherd codiscovered the first known solar-system-size disk around a massive star five years ago, and nearly a dozen such systems now are known, including the famous Becklin-Neugebauer object, a once-mysterious infrared source hidden in the depths of the Orion Nebula, whose newfound disk also appears in this week's Nature. But Cepheus A HW2 "is one of the best single examples," says Shepherd, "and it supports a growing consensus that even the most massive stars form by accretion."