Outbursts of young stellar objects [PDF]
Monthly Notices of the Royal Astronomical Society, 2004 We argue that the outbursts of the FU Orionis stars occur on timescales which are much longer than expected from the standard disc instability model with _{c} \gtrsim 10^{-3}. The outburst, recurrence, and rise times are consistent with the idea that the accretion disc in these objects is truncated at a radius R_{i} \sim 40 \rsun. In agreement with a
Matthews, OM, Speith, R, Wynn, GA
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Kinematics of Young Stellar Objects under Various Stellar Feedback
The Astrophysical Journal Supplement SeriesBased on the Gaia Data Release 3 and APOGEE data sets, we investigate the kinematic differences between young stellar objects (YSOs) and their parent clouds in five nearby star-forming regions.
Longhui Yang +8 more
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CO Outflows from Young Stellar Objects [PDF]
The Astrophysical Journal, 2002 We have mapped the CO J = 1-0 emission from molecular outflows associated with six young stellar systems using the BIMA array. The systems are all relatively nearby, have low-luminosity, and range from Class 0 to Class II sources. The CO outflows in these systems are complicated, showing multipolar structures, multiple cavities, and asymmetric lobes ...
Chin‐Fei Lee +3 more
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YSOVAR: mid-infrared variability of young stellar objects and their disks in the cluster IRAS 20050+2720 [PDF]
, 2015 We present a time-variability study of young stellar objects (YSOs) in the cluster IRAS 20050+2720, performed at 3.6 and 4.5 μm with the Spitzer Space Telescope; this study is part of the Young Stellar Object VARiability (YSOVAR) project.
Katja Poppenhaeger +14 more
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A CLASSIFICATION SCHEME FOR YOUNG STELLAR OBJECTS USING THEWIDE-FIELD INFRARED SURVEY EXPLORERAllWISE CATALOG: REVEALING LOW-DENSITY STAR FORMATION IN THE OUTER GALAXY [PDF]
, 2014 We present an assessment of the performance of WISE and the AllWISE data release for a section of the Galactic Plane. We lay out an approach to increasing the reliability of point-source photometry extracted from the AllWISE catalog in Galactic Plane ...
X. P. Koenig, D. T. Leisawitz
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Complex organic molecules in organic-poor massive young stellar objects [PDF]
, 2015 Massive young stellar objects (MYSOs) with hot cores are classic sources of complex organic molecules. The origins of these molecules in such sources, as well as the small- and large-scale differentiation between nitrogen- and oxygen-bearing complex ...
Edith C. Fayolle +4 more
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X-shooter spectroscopy of young stellar objects. IV. Accretion in low-mass stars and substellar objects in Lupus [PDF]
, 2013 We present X-Shooter/VLT observations of a sample of 36 accreting low-mass stellar and sub-stellar objects (YSOs) in the Lupus star forming region, spanning a range in mass from ~0.03 to ~1.2Msun, but mostly with 0.1Msun < Mstar < 0.5Msun.
J. Alcal'a +15 more
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X-shooter spectroscopy of young stellar objects [PDF]
, 2013 Context. The lack of knowledge of photospheric parameters and the level of chromospheric activity in young low-mass pre-main sequence stars introduces uncertainties when measuring mass accretion rates in accreting (Class II) Young Stellar Objects.
B. Stelzer +9 more
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Infrared Nebulae around Young Stellar Objects [PDF]
The Astronomical Journal, 2007 79 pages, 33 ...
Connelley, Michael S. +2 more
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X-shooter spectroscopy of young stellar objects in Lupus [PDF]
Astronomy & Astrophysics, 2017 With the purpose of performing a homogeneous determination of elemental abundances for members of the Lupus T association, we analyzed three chemical elements: lithium, iron, and barium.
K. Biazzo +11 more
semanticscholar +1 more source