Published in

Astronomy & Astrophysics, (591), p. L3, 2016

DOI: 10.1051/0004-6361/201628549

Links

Tools

Export citation

Search in Google Scholar

Evidence for a correlation between mass accretion rates onto young stars and the mass of their protoplanetary disks

This paper was not found in any repository, but could be made available legally by the author.
This paper was not found in any repository, but could be made available legally by the author.

Full text: Unavailable

Green circle
Preprint: archiving allowed
Green circle
Postprint: archiving allowed
Green circle
Published version: archiving allowed
Data provided by SHERPA/RoMEO
Beta version