84 citations · 143 across the 5 of their papers we have counts for
6 papers
Characteristics of small protoplanetary disc warps in kinematic observations
Alison K. Young, Richard Alexander, Giovanni Rosotti +1
Many circumstellar discs appear to have misaligned central regions that give rise to shadows seen in scattered light observations. Small warps ( misalignment) are probab…
Chemical signatures of a warped protoplanetary disc
Alison K. Young, Richard Alexander, Catherine Walsh +3
Circumstellar discs may become warped or broken into distinct planes if there is a stellar or planetary companion with an orbit that is misaligned with respect to the disc. There i…
A triple star system with a misaligned and warped circumstellar disk shaped by disk tearing
Stefan Kraus, Alexander Kreplin, Alison K. Young +29
Young stars are surrounded by a circumstellar disk of gas and dust, within which planet formation can occur. Gravitational forces in multiple star systems can disrupt the disk. The…
Synthetic molecular line observations of the first hydrostatic core from chemical calculations
Alison K. Young, Matthew R. Bate, Tim J. Harries +1
The first stable object to develop in the low-mass star formation process has long been predicted to be the first hydrostatic core (FHSC). Despite much effort, it has still yet to…
Dust-trapping vortices and a potentially planet-triggered spiral wake in the pre-transitional disk of V1247 Orionis
Stefan Kraus, Alexander Kreplin, Misato Fukagawa +8
The radial drift problem constitutes one of the most fundamental problems in planet formation theory, as it predicts particles to drift into the star before they are able to grow t…
What can the SEDs of first hydrostatic core candidates reveal about their nature?
Alison K. Young, Matthew R. Bate, Chris F. Mowat +2
The first hydrostatic core (FHSC) is the first stable object to form in simulations of star formation. This stage has yet to be observed definitively, although several candidate FH…