Zobrazeno 1 - 10
of 433
pro vyhledávání: '"FU Orionis stars"'
Autor:
Dullemond, Cornelis Petrus, Küffmeier, Michael, Goicovic, Felipe, Fukagawa, Misato, Oehl, Veronika, Kramer, Manuel
Publikováno v:
Astronomy and Astrophysics, 628, 20 (2019)
After its formation, a young star spends some time traversing the molecular cloud complex in which it was born. It is therefore not unlikely that, well after the initial cloud collapse event which produced the star, it will encounter one or more low
Externí odkaz:
http://arxiv.org/abs/1911.05158
FU Orionis stars (FUORS) are eruptive pre-main sequence objects thought to represent quasi-periodic or recurring stages of enhanced accretion during the low-mass star-forming process. We characterize the sample of known and candidate FUORS in an homo
Externí odkaz:
http://arxiv.org/abs/1402.3240
Publikováno v:
Astrophys.J.658:487-497,2007
We present Spitzer IRAC and IRS observations of the dark cloud L1287. The mid-infrared (MIR) IRAC images show deeply embedded infrared sources in the vicinity of the FU Orionis objects RNO 1B and RNO 1C suggesting their association with a small young
Externí odkaz:
http://arxiv.org/abs/astro-ph/0612096
Autor:
GOODRICH, ROBERT W.
Publikováno v:
Publications of the Astronomical Society of the Pacific, 1987 Feb 01. 99(612), 116-125.
Externí odkaz:
https://www.jstor.org/stable/40678875
Autor:
LANDOLT, ARLO U.
Publikováno v:
Publications of the Astronomical Society of the Pacific, 1977 Oct 01. 89(531), 704-705.
Externí odkaz:
https://www.jstor.org/stable/40677095
Publikováno v:
Publications of the Astronomical Society of the Pacific, 1990 Dec 01. 102(658), 1413-1417.
Externí odkaz:
https://www.jstor.org/stable/40679646
Akademický článek
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Publikováno v:
The Astrophysical Journal Letters, Vol 973, Iss 2, p L40 (2024)
FU Ori objects are the most extreme eruptive young stars known. Their 4–5 mag photometric outbursts last for decades and are attributed to a factor of up to 10,000 increase in the stellar accretion rate. The nature of the accretion disk-to-star int
Externí odkaz:
https://doaj.org/article/1ccc446bc1934ace9de6feb8caa1ccdd
Autor:
Misato Fukagawa, Veronika Oehl, F. G. Goicovic, M. Kuffmeier, Manuel Kramer, Cornelis P. Dullemond
After its formation, a young star spends some time traversing the molecular cloud complex in which it was born. It is therefore not unlikely that, well after the initial cloud collapse event which produced the star, it will encounter one or more low
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::6ff97ad90bb0e50d69d9b709e72af8ae
Akademický článek
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