A dusty pinwheel nebula around the massive star WR 104

@misc{citeulike:2463854, abstract = {m respectively) for both observing epochs. As infrared emission from the hot circumstellar dust dominates the infrared region of the spectrum, we may interpret the highly asymmetric curved plumes evident in the maps as tracing the distribution of this material. Previous high-resolution efforts have been restricted to partially-resolved one-dimensional visibility curves interpreted in the context of spherically symmetric outflow models [7, 8]. As a comparison with these earlier results, we have...}, author = {John, Peter T. }, citeulike-article-id = {2463854}, keywords = {astronomy, gammaraybursts, grb}, posted-at = {2008-03-04 10:31:34}, priority = {0}, title = {A dusty pinwheel nebula around the massive star WR 104}, url = {http://citeseer.ist.psu.edu/497021.html} }

TY - GEN ID - citeulike:2463854 L3 - citeulike-article-id:2463854 TI - A dusty pinwheel nebula around the massive star WR 104 N2 - m respectively) for both observing epochs. As infrared emission from the hot circumstellar dust dominates the infrared region of the spectrum, we may interpret the highly asymmetric curved plumes evident in the maps as tracing the distribution of this material. Previous high-resolution efforts have been restricted to partially-resolved one-dimensional visibility curves interpreted in the context of spherically symmetric outflow models [7, 8]. As a comparison with these earlier results, we have... KW - astronomy KW - gammaraybursts KW - grb AU - John, Peter UR - http://citeseer.ist.psu.edu/497021.html ER -