Anneila I. Sargent
California Institute of Technology
156 Papers
2.1K Citations
Anneila I. Sargent is an academic researcher from California Institute of Technology. The author has contributed to research in topics: Star formation & T Tauri star. The author has an hindex of 63, co-authored 156 publications.
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Papers
The FU Orionis binary system RNO 1B/1C
TL;DR: In this paper, high spatial resolution interferometer observations of CS (2→1) emission may trace the dense walls of the Orionis outflow cavity comprised of two concentric arcs with dynamical ages of 4×10^3 and 1 ×10^4 yr.
Anatomy of a merger : CO in Arp 299 (IC 694-NGC 3690)
Anneila I. Sargent,Nick Scoville +1 more
TL;DR: In this article, high-resolution CO observations of the interacting system Arp 299 (Mrk 171: IC 694 and NGC 3690) reveal major gas condensations at the nuclei of both galaxies and in the disk overlap region.
Interacting coronae of two T Tauri stars: first observational evidence for solar-like helmet streamers
M. Massi,Eduardo Ros,Karl M. Menten,M. M. Kaufman Bernado,G. Torricelli-Ciamponi,J. Neidhöfer,Andrew F. Boden,D. A. Boboltz,Anneila I. Sargent,Guillermo Torres +9 more
TL;DR: In this article, the authors show that even if the radio flaring origin is magnetic reconnection due to interbinary collision, both stars independently emit in the radio range with structures of their own.
The Spitzer c2d Survey of Large, Nearby, Insterstellar Clouds. II. Serpens Observed with IRAC
Paul M. Harvey,Nicholas Chapman,Shih-Ping Lai,Neal J. Evans,Lori Allen,Jes K. Jørgensen,Lee G. Mundy,Tracy L. Huard,A. Porras,Lucas A. Cieza,Philip C. Myers,Bruno Merín,Ewine F. van Dishoeck,Kaisa E. Young,William Spiesman,Geoffrey A. Blake,David W. Koerner,Deborah Padgett,Anneila I. Sargent,Karl R. Stapelfeldt +19 more
TL;DR: In this article, the authors present maps of the Serpens dark cloud at 3.6, 4.5, 5.8, and 8.0?m observed with the Spitzer Space Telescope Infrared Array Camera (IRAC).
Disk Mass Limits and Lifetimes of Externally Irradiated Young Stellar Objects Embedded in the Orion Nebula
TL;DR: In this article, the authors presented 1.3 mm wavelength interferometric observations of externally irradiated young stellar objects (proplyds) embedded within the Orion Nebula, including the three largest circumstellar disks seen in silhouette against the background nebular light.