Results 91 to 100 of about 2,019 (232)
Cloud Dissipation and Disk Wind in the Late Phase of Star Formation
The Astrophysical JournalWe perform a long-term simulation of star and disk formation using three-dimensional nonideal magnetohydrodynamics. The simulation starts from a prestellar cloud and proceeds through the long-term evolution of the circumstellar disk until ∼1.5 × 10 ^5 yr
Masahiro N. Machida, Shantanu Basu
doaj +1 more source
SPECKLE SUPPRESSION THROUGH DUAL IMAGING POLARIMETRY, AND A GROUND-BASED IMAGE OF THE HR 4796A CIRCUMSTELLAR DISK [PDF]
, 2009 Sasha Hinkley +9 more
openalex +1 more source
Spectropolarimetry and the Study of Circumstellar Disks [PDF]
, 2007 Circumstellar disks play an important role in many stages of the evolution of stars. However, it is only possible to directly image circumstellar disks for a few of the nearest stars. For massive stars, the situation is even more difficult, as they are on average further away than the more numerous low mass stars.
openaire +2 more sources
Phosphorus-bearing molecules PO and PN at the edge of the Galaxy. [PDF]
Nature, 2023 Koelemay LA, Gold KR, Ziurys LM.
europepmc +1 more source
Indicator of Exo-Solar Planet(s) in the Circumstellar Disk Around β Pictoris [PDF]
, 2004 Nick Gorkavyi +4 more
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GANBISS: a new GPU accelerated N-body code for binary star systems. [PDF]
Celest Mech Dyn Astron, 2023 Zimmermann M, Pilat-Lohinger E.
europepmc +1 more source
86th Annual Meeting of the Meteoritical Society (2024)
Meteoritics &Planetary Science, Volume 59, Issue S1, Page A1-A468, August 2024.
wiley +1 more source
The Astrophysical JournalThe discovery of protoplanets and circumplanetary disks provides a unique opportunity to characterize planet formation through observations. Massive protoplanets shape the physical and chemical structure of their host circumstellar disk by accretion ...
Felipe Alarcón, Edwin A. Bergin
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Identification of Possible Stellar Companions via Speckle Interferometry in a Sample of Be Stars II
The Astronomical JournalThis study investigates the identification of possible stellar companions in a sample of Be stars using speckle interferometry. Be stars, which are rapidly rotating B-type stars exhibiting emission lines due to the presence of circumstellar disks, have ...
C. A. Guerrero +3 more
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