Accretion, outflows, and winds of magnetized stars
MM Romanova, SP Owocki - Space Science Reviews, 2015 - Springer
Many types of stars have strong magnetic fields that can dynamically influence the flow of
circumstellar matter. In stars with accretion disks, the stellar magnetic field can truncate the …
circumstellar matter. In stars with accretion disks, the stellar magnetic field can truncate the …
[HTML][HTML] Probing inner and outer disk misalignments in transition disks-Constraints from VLTI/GRAVITY and ALMA observations
AJ Bohn, M Benisty, K Perraut, N van Der Marel… - Astronomy & …, 2022 - aanda.org
Context. Transition disks are protoplanetary disks with dust-depleted cavities, possibly
indicating substantial clearing of their dust content by a massive companion. For several …
indicating substantial clearing of their dust content by a massive companion. For several …
Episodic accretion in young stars
M Audard, P Abrahám, MM Dunham… - … and planets VI, 2014 - books.google.com
Episodic accretion has become a recent focus of attention in the star-and planet-formation
community, turning into a central topic to understand the evolution of protostars and …
community, turning into a central topic to understand the evolution of protostars and …
CSI 2264: simultaneous optical and infrared light curves of young disk-bearing stars in NGC 2264 with CoRoT and Spitzer—evidence for multiple origins of variability
AM Cody, J Stauffer, A Baglin, G Micela… - The Astronomical …, 2014 - iopscience.iop.org
ABSTRACT We present the Coordinated Synoptic Investigation of NGC 2264, a continuous
30 day multi-wavelength photometric monitoring campaign on more than 1000 young cluster …
30 day multi-wavelength photometric monitoring campaign on more than 1000 young cluster …
A survey and analysis of Spitzer infrared spectrograph spectra of T Tauri stars in Taurus
E Furlan, L Hartmann, N Calvet… - The Astrophysical …, 2006 - iopscience.iop.org
We present mid-infrared spectra of T Tauri stars in the Taurus star-forming region obtained
with the Spitzer Infrared Spectrograph (IRS). For the first time, the 5-36 μm spectra of a large …
with the Spitzer Infrared Spectrograph (IRS). For the first time, the 5-36 μm spectra of a large …
Magnetospheric accretion in classical T Tauri stars
J Bouvier, SHP Alencar, TJ Harries… - arXiv preprint astro-ph …, 2006 - arxiv.org
The inner 0.1 AU around accreting T Tauri stars hold clues to many physical processes that
characterize the early evolution of solar-type stars. The accretion-ejection connection takes …
characterize the early evolution of solar-type stars. The accretion-ejection connection takes …
Ysovar: the first sensitive, wide-area, mid-infrared photometric monitoring of the Orion Nebula Cluster
M Morales-Calderón, JR Stauffer… - The Astrophysical …, 2011 - iopscience.iop.org
We present initial results from time-series imaging at infrared wavelengths of 0.9 deg 2 in the
Orion Nebula Cluster (ONC). During Fall 2009 we obtained 81 epochs of Spitzer 3.6 and 4.5 …
Orion Nebula Cluster (ONC). During Fall 2009 we obtained 81 epochs of Spitzer 3.6 and 4.5 …
Magnetospheric accretion-ejection processes in the classical T Tauri star AA Tauri
J Bouvier, SHP Alencar, T Boutelier… - Astronomy & …, 2007 - aanda.org
Context. Accretion and ejection are complex and related processes that vary on various
timescales in young stars. Aims. We intend to investigate the accretion and outflow dynamics …
timescales in young stars. Aims. We intend to investigate the accretion and outflow dynamics …
Three-dimensional simulations of disk accretion to an inclined dipole. II. Hot spots and variability
MM Romanova, GV Ustyugova… - The Astrophysical …, 2004 - iopscience.iop.org
The physics of the hot spots on stellar surfaces and the associated variability of accreting
magnetized rotating stars is investigated for the first time using fully three-dimensional …
magnetized rotating stars is investigated for the first time using fully three-dimensional …
Three-dimensional simulations of disk accretion to an inclined dipole. I. Magnetospheric flows at different Θ
MM Romanova, GV Ustyugova… - The Astrophysical …, 2003 - iopscience.iop.org
We present results of fully three-dimensional MHD simulations of disk accretion to a slowly
rotating magnetized star with its dipole moment inclined at an angle Θ to the rotation axis of …
rotating magnetized star with its dipole moment inclined at an angle Θ to the rotation axis of …