Results 91 to 100 of about 64,867 (203)
Weakened Magnetic Braking Signals the Collapse of the Global Stellar Dynamo
Weakened magnetic braking (WMB) was originally proposed in 2016 to explain anomalously rapid rotation in old field stars observed by the Kepler mission.
Travis S. Metcalfe +9 more
doaj +1 more source
Stellar winds driven by Alfven waves [PDF]
Models of stellar winds were considered in which the dynamic expansion of a corona is driven by Alfven waves propagating outward along radial magnetic field lines.
Belcher, J. W., Olbert, S.
core +1 more source
Observations of Extremely Metal-poor O Stars: Weak Winds and Constraints for Evolution Models
Metal-poor massive stars drive the evolution of low-mass galaxies, both locally and at high redshift. However, quantifying the feedback they impart to their local surroundings remains uncertain because models of stellar evolution, mass loss, and ionizing
O. Grace Telford +5 more
doaj +1 more source
Lyman alpha initiated winds in late-type stars [PDF]
The IUE survey of late-type stars revealed a sharp division in the HR diagram between stars with solar type spectra (chromosphere and transition region lines) and those with non-solar type spectra (only chromosphere lines). Models of both hot coronae and
Haisch, B. M. +2 more
core +1 more source
The removal of angular momentum from protostellar systems drives accretion onto the central star and may drive the dispersal of the protoplanetary disk. Winds and jets can contribute to removing angular momentum from the disk, though the dominant process
Kamber R. Schwarz +23 more
doaj +1 more source
Stellar-wind-blown Bubbles as Environments for Late-time Rebrightening of Gamma-ray Burst Afterglows
We present multiwavelength afterglow fitting results for three events that exhibit late afterglow rebrightening behavior: EP240414a ( z = 0.401), GRB 240529A ( z = 2.695), and GRB 240218A ( z = 6.782), which span a broad range of redshifts, from the ...
Jia Ren +7 more
doaj +1 more source
Investigating Protostellar Accretion is a Cycle 1 JWST program using the NIRSpec+MIRI integral field units to obtain 2.9–28 μ m spectral cubes of five young protostars with luminosities of 0.2–10,000 L _⊙ in their primary accretion phase.
Samuel A. Federman +38 more
doaj +1 more source
Measuring the magnetic fields in the chromospheres of low-mass stars [PDF]
Cang T +13 more
europepmc +2 more sources
A Study of Emission Lines in Carbon Stars
Carbon stars are chemically peculiar stars with high carbon abundance, showing strong carbon molecule bands and rare emission lines in their spectra. This paper explores the stellar activity of carbon stars by identifying emission line features in their ...
Lichan Zhou +5 more
doaj +1 more source
PROJECT-J: The Shocking H2 Outflow from HH 46
We analyze the H _2 emission observed in the HH 46 Class I system as part of PROtostellar JEts Cradle Tested with JWST (PROJECT-J), to investigate the origin and excitation of the warm molecular outflow. We used NIRSpec and MIRI spectral maps (1.6–27.9 μ
Maria Gabriela Navarro +16 more
doaj +1 more source

