Dust Morphology and Composition in FU Orionis Systems-Reference-Cited by-同舟云学术

Dust Morphology and Composition in FU Orionis Systems

Published:2005-02 Issue:2 Volume:129 Page:1035-1048
ISSN:0004-6256
Container-title:The Astronomical Journal
language:en
Short-container-title:Astron J

Author:

Polomski E. F.,Woodward Charles E.,Holmes Elizabeth K.,Butner Harold M.,Lynch David K.,Russell Ray W.,Sitko Michael L.,Wooden Diane H.,Telesco C. M.,Piña R.

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Reference110 articles.

1. Long-term evolution of FU Orionis objects at infrared wavelengths

2. A radio candidate for the exciting source of the L1287 bipolar outflow

3. Parameters of disks around young stellar objects from polarization observations

4. An ISO investigation of the MWC 297 circumstellar region

5. Infrared emission from dust structures surrounding Herbig Ae/Be stars

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2. The ALMA early science view of FUor/EXor objects – V. Continuum disc masses and sizes;Monthly Notices of the Royal Astronomical Society;2017-11-27

3. SPECTRAL ENERGY DISTRIBUTION ANALYSIS OF CLASS I AND CLASS II FU ORIONIS STARS;The Astronomical Journal;2014-05-06

4. Mineralogical study of proto-planetary disks in FU Orionis stars;Proceedings of the International Astronomical Union;2009-11

5. High-resolution polarimetry of Parsamian 21: revealing the structure of an edge-on FU Ori disc★;Monthly Notices of the Royal Astronomical Society;2008-01-09