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VLBI observations of two 43-GHz SiO masers in R Cas

VLBI observations of two 43-GHz SiO masers in R Cas

VLBI observations of two 43-GHz SiO masers in R Cas. Jiyune Yi Korea VLBI Network ( KVN ) group Korea Astronomy and Space Science Institute In collaboration with R. Booth 1,2 and J. Conway 1 1. Onsala Space Observatory, Sweden 2. Hartebeesthoek Radio Astronomy Observatory.

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397 views • 27 slides
KVN

KVN

KVN. Advances in Source/Frequency Phase Referencing with KVN Astrometric comparison of sites of maser emission in R Leo Minoris. Richard Dodson: Brain Pool Fellow@KASI. KVN observations of R Leo Min.

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352 views • 21 slides
mmVLBI in the Future: technical/experimental

mmVLBI in the Future: technical/experimental

mmVLBI in the Future: technical/experimental. Shep Doeleman Haystack Observatory. In Defense of Theory. Do I contradict myself? Very well then I contradict myself, (I am large, I contain multitudes.) --Walt Whitman, "Song of Myself". High Frequency VLBI Challenges.

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313 views • 19 slides
CIRIACO GODDI European Southern Observatory

CIRIACO GODDI European Southern Observatory

Disk-mediated accretion in a high-mass YSO and dynamical history in Orion BN/KL. CIRIACO GODDI European Southern Observatory. Main collaborators Lincoln Greenhill Harvard-Smithsonian Center for Astrophysics Lynn Matthews MIT Haystack Observatory Liz Humphreys

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413 views • 16 slides
???????? VLBI ????? ?????????????? ???

???????? VLBI ????? ?????????????? ???

?? VLBI ??????? VLBI ?????????? 2010 ? 11 ? 12 ?. ???????? VLBI ????? ?????????????? ???. Hiroshi Imai Graduate School of Science and Engineering Kagoshima University. Contents: Proposal as an EAVN key science project. What can we learn from stellar masers? Current trial observations

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413 views • 14 slides
VLBA SiO Maser Observations of the OH/IR Star OH 44.8-2.3: Magnetic Field and Morphology

VLBA SiO Maser Observations of the OH/IR Star OH 44.8-2.3: Magnetic Field and Morphology

VLBA SiO Maser Observations of the OH/IR Star OH 44.8-2.3: Magnetic Field and Morphology. Huib Jan van Langevelde (JIVE/ Leiden Observatory) Wouter Vlemmings (Chalmers University) Athol Kemball (University of Illinois). Nikta Amiri (University of Colorado Boulder). TX Cam (73 Epochs).

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141 views • 14 slides
mm VLBI: World Record Resolution and Study of SiO Masers

mm VLBI: World Record Resolution and Study of SiO Masers

I. Why push the VLBI technique to shorter wavelengths?. Better resolution ( l /D). b. Faraday rotation and, thus, depolarization in quasar cores decreases as l 2 . c. Scatter broadening through ionized media decreases as l 2 .

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90 views • 1 slides

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