M. Goto et al. 2006 ApJ 652 758 doi:10.1086/506582
M. Goto1, T. Usuda2, C. P. Dullemond1, Th. Henning1, H. Linz1,3, B. Stecklum3 and H. Suto4
Show affiliationsWe present high-resolution infrared spectroscopy of the Herbig Ae star HD 141569A in the CO v = 2-1 transition. With the angular resolution attained by the adaptive optics system, the gas disk around HD 141569A is spatially resolved down to its inner-rim truncation. The size of the inner clearing is 11 ± 2 AU in radius, close to the gravitational radius of the star. The rough coincidence with the gravitational radius indicates that the viscous accretion working together with photoevaporation by stellar radiation has cleared the inner part of the disk.
circumstellar matter; infrared: stars; planetary systems: formation; planetary systems: protoplanetary disks; stars: formation; stars: individual (HD 141569A)
Issue 1 (2006 November 20)
Received 2005 December 12, accepted for publication 2006 June 8
M. Goto et al. 2006 ApJ 652 758
Gernot J Pauschenwein and Gerhard Kahl 2009 J. Phys.: Condens. Matter 21 474202
Feng Qiao et al 2006 Phys. Med. Biol. 51 3769
M T Batchelor et al 2005 J. Phys. A: Math. Gen. 38 7787
A Bashir and R Delbourgo 2004 J. Phys. A: Math. Gen. 37 6587
Shi-shyr Roan 2006 J. Phys. A: Math. Gen. 39 12303
Reinout Quispel and Robert McLachlan 2006 J. Phys. A: Math. Gen. 39
S G Whittington and A J Guttmann 1990 J. Phys. A: Math. Gen. 23 5601
Asghar Ramezani and Aria Alasty 2009 J. Phys. D: Appl. Phys. 42 225506
Stacy H. Teng et al. 2005 ApJ 633 664