Shadow of a forming star

In March 2008 the scientists observed the young star (protostar) system 2M171123 in the B59 molecular cloud, with the Cerro Tololo Inter-American Observatory (CTIO) 4-m telescope in Chile. They found an odd feature in their image - a shadowed dark lane just to the west of the protostar with a thickness of about 54 billion kilometres (360 times the distance from the Earth to the Sun).

Silhouetted images of young star systems and the disks that often surround them (some of which will go on to form planets) are common. But interestingly, in this case the shadow is offset from the protostar, and the offset has been confirmed by comparing the position of this system in the CTIO observations by another at infrared wavelengths from the NASA Spitzer Space Telescope.

Explaining their result, the team suggests a scenario in which the protostar casts its shadow onto a nearby background cloud of material. A scattering cloud that lies offset from the star acts as a screen onto which its shadow is projected. The team has also confirmed that this is not an edge-on disk, but a system viewed at an intermediate inclination.

This is thus an interesting new observation of an offset shadowed lane among young stellar objects. In the future the team plan to obtain images of the system at higher resolution and look out for any variability in the shadowed lane over time.

Provided by Royal Astronomical Society (news : web)