We present results of the Mt Abu JHK photometric and HI Brackett γ line monitoring of the eruptive young stellar object V1647 Orionis （McNeil＇s Object） during its ongoing outburst phase in 2008-2012. We discuss JH...We present results of the Mt Abu JHK photometric and HI Brackett γ line monitoring of the eruptive young stellar object V1647 Orionis （McNeil＇s Object） during its ongoing outburst phase in 2008-2012. We discuss JHK color patterns and extinction during the outburst and compare them with those from the previous out- burst phase in 2004-2005 and in the intervening quiescent period that lasted about 2 yr. Commencing from early 2012, the object has shown a slow fading out in all the bands. We report brightness variations in the nearby Herbig-Haro object HH22 that are possibly associated with those in V1647 Ori. We also present modeling of the spec- tral energy distributions of V 1647 Ori during both its recent outburst and its quiescent phase. The physical parameters of the protostar and its circumstellar environment ob- tained from the modeling indicate marked differences between the two phases.展开更多
基金supported by the Department of Space Government of India
文摘We present results of the Mt Abu JHK photometric and HI Brackett γ line monitoring of the eruptive young stellar object V1647 Orionis （McNeil＇s Object） during its ongoing outburst phase in 2008-2012. We discuss JHK color patterns and extinction during the outburst and compare them with those from the previous out- burst phase in 2004-2005 and in the intervening quiescent period that lasted about 2 yr. Commencing from early 2012, the object has shown a slow fading out in all the bands. We report brightness variations in the nearby Herbig-Haro object HH22 that are possibly associated with those in V1647 Ori. We also present modeling of the spec- tral energy distributions of V 1647 Ori during both its recent outburst and its quiescent phase. The physical parameters of the protostar and its circumstellar environment ob- tained from the modeling indicate marked differences between the two phases.
