LINKING CHEMISTRY AND KINEMATICS IN THE MOLECULAR GAS OF PROTOPLANETARY NEBULA M1-92 [PDF]
. Protoplanetary nebulae (PPNe) play a significant role in the evolution of low and intermediate mass stars, serving as the link between the asymptotic giant branch (AGB) and planetary nebulae phases.
Katherine J. Gold, L. M. Ziurys
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Oxygen Isotope Constraints on the Importance of Photochemical Processing in Protoplanetary Disks
Observations have revealed evidence of photochemical processing in protoplanetary disks. This processing occurs in the photon-dominated layer, the optically thin regions of the disk high above the disk midplane. It remains unclear, however, how much this
Fred J. Ciesla +3 more
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Millimetre polarization of the protoplanetary nebula OH 231.8+4.2: a follow-up study with CARMA [PDF]
In order to investigate the characteristics and influence of the magnetic field in evolved stars, we performed a follow-up investigation of our previous submillimeter analysis of the proto-planetary nebula (PPN) OH 231.8+4.2 (Sabin et al.
L. Sabin +6 more
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ALMA Observations of Asymmetric Molecular Gas Emission from a Protoplanetary Disk in the Orion Nebula [PDF]
We present Atacama Large Millimeter/submillimeter Array (ALMA) observations of molecular line emission from d216-0939, one of the largest and most massive protoplanetary disks in the Orion Nebula Cluster.
Samuel M. Factor +9 more
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HST STIS UV Spectroscopic Observations of the Protoplanetary Nebula Hen3-1475∗ † [PDF]
We present UV spectra of the protoplanetary nebula (pPN) Hen 3-1475 obtained with the Space Telescope Imaging Spectrograph (STIS) on board the Hubble Space Telescope (HST). Our deep, low-dispersion spectroscopy enables monochromatic imaging of Hen 3-1475
Xuan Fang +3 more
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Early science with the Large Millimeter Telescope: molecules in the extreme outflow of a protoplanetary nebula [PDF]
Extremely high velocity emission likely related to jets is known to occur in some proto-Planetary Nebulae. However, the molecular complexity of this kinematic component is largely unknown.
Arturo I. Gómez-Ruiz +13 more
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Discovery of Radio Recombination Lines from Proplyds in the Orion Nebula Cluster
We present new Atacama Large Millimeter/submillimeter Array observations that, for the first time, detect hydrogen and helium radio recombination lines from a protoplanetary disk.
Ryan D. Boyden +7 more
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Size-selective concentration of chondrules and other small particles in protoplanetary nebula turbulence [PDF]
Size-selective concentration of particles in a weakly turbulent protoplanetary nebula may be responsible for the initial collection of chondrules and other constituents into primitive body precursors. This paper presents the main elements of this process
Barge P. +23 more
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Particle confinement in a non-axisymmetric protoplanetary nebula
Fuente Marcos C. de la, Barge P.
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DETECTION OF C60IN THE PROTOPLANETARY NEBULA IRAS 01005+7910 [PDF]
We report the first detection of buckminsterfullerene (C60) in a protoplanetary nebula. The vibrational transitions of C60 at 7.0, 17.4, and 18.9 μm are detected in the Spitzer/Infrared Spectrograph spectrum of IRAS 01005+7910.
Yong Zhang, Sun Kwok
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