THE FU ORIONIS PHENOMENON
- 1 September 1996
- journal article
- Published by Annual Reviews in Annual Review of Astronomy and Astrophysics
- Vol. 34 (1) , 207-240
- https://doi.org/10.1146/annurev.astro.34.1.207
Abstract
No abstract availableKeywords
This publication has 87 references indexed in Scilit:
- Disk Accretion and Mass Loss from Young StarsThe Astrophysical Journal, 1995
- Identification of Ionizing Sources and Young Stellar Objects in M17The Astrophysical Journal, 1995
- Disks in pre-main sequence starsAstrophysics and Space Science, 1995
- A parsec-scale 'superjet' and quasi-periodic structure in the HH 34 outflow?The Astrophysical Journal, 1994
- Near-infrared spectrophotometry of FU Orionis variablesThe Astrophysical Journal, 1992
- Are FU Orionis stars younger than T Tauri stars? Submillimeter constraints on circumstellar disksThe Astrophysical Journal, 1991
- Rotational and radial velocities of T Tauri starsThe Astrophysical Journal, 1986
- The optical spectrum of L1551 IRS 5The Astrophysical Journal, 1985
- Spectroscopic and photometric observations of the Herbig Be star Z Canis MajorisThe Astronomical Journal, 1984
- Photometric histories of six infrared objects and three highly reddened blue supergiantsThe Astrophysical Journal, 1978