Theory predicts and observations confirm that low-mass stars (like the Sun) in their early life grow by accreting gas from the surrounding material. But for stars ~10 times more massive than the Sun (~10Msolar), the powerful stellar radiation is expected to inhibit accretion and thus limit the growth of their mass. Clearly, stars with masses >10Msolar exist, so there must be a way for them to form. The problem may be solved by non-spherical accretion, which allows some of the stellar photons to escape along the symmetry axis where the density is lower. The recent detection of rotating disks and toroids around very young massive stars has lent support to the idea that high-mass (>~8Msolar) stars could form in this way. Here we report observations of an ammonia line towards a high-mass star forming region. We conclude that the gas is falling inwards towards a very young star of ~20Msolar, in line with theoretical predictions of non-spherical accretion.
BELTRN M.T, CESARONI R, CODELLA C, TESTI L, FURUYA R.S, OLMI L (2006). Infall of gas as the formation mechanism of stars up to 20 times more massive than the Sun. NATURE, 443, 427-429 [10.1038/nature05074].
Infall of gas as the formation mechanism of stars up to 20 times more massive than the Sun
TESTI L;
2006
Abstract
Theory predicts and observations confirm that low-mass stars (like the Sun) in their early life grow by accreting gas from the surrounding material. But for stars ~10 times more massive than the Sun (~10Msolar), the powerful stellar radiation is expected to inhibit accretion and thus limit the growth of their mass. Clearly, stars with masses >10Msolar exist, so there must be a way for them to form. The problem may be solved by non-spherical accretion, which allows some of the stellar photons to escape along the symmetry axis where the density is lower. The recent detection of rotating disks and toroids around very young massive stars has lent support to the idea that high-mass (>~8Msolar) stars could form in this way. Here we report observations of an ammonia line towards a high-mass star forming region. We conclude that the gas is falling inwards towards a very young star of ~20Msolar, in line with theoretical predictions of non-spherical accretion.I documenti in IRIS sono protetti da copyright e tutti i diritti sono riservati, salvo diversa indicazione.
