Precise measurements by the ESO instrument HARPS now show that the rotation of the Milky Way is simpler than previously thought - the much debated, apparent 'fall' of neighborhood Cepheid stars towards our Sun stems from an intrinsic property of the Cepheids themselves, say a group of astrophysicists led by Nicolas Nardetto in a Astronomy & Astrophysics article.
Since Henrietta Leavitt's discovery of their unique properties in 1912, the class of bright, pulsating stars known as Cepheids has been used as a distance indicator. Combined with velocity measurements, the properties of Cepheids are also an extremely valuable tool in investigations of how our galaxy, the Milky Way, rotates.
"The motion of Milky Way Cepheids is confusing and has led to disagreement among researchers," says Nardetto. "If the rotation of the Galaxy is taken into account, the Cepheids appear to 'fall' towards the Sun with a mean velocity of about 2 km/s."