38 citations · 114 across the 7 of their papers we have counts for
7 papers
A survey for variable young stars with small telescopes: IV -- Rotation Periods of YSOs in IC5070
Dirk Froebrich, Efthymia Derezea, Aleks Scholz +50
Studying rotational variability of young stars is enabling us to investigate a multitude of properties of young star-disk systems. We utilise high cadence, multi-wavelength optical…
A survey for variable young stars with small telescopes: II -- Mapping a protoplanetary disk with stable structures at 0.15 AU
Jack J. Evitts, Dirk Froebrich, Aleks Scholz +57
The HOYS citizen science project conducts long term, multifilter, high cadence monitoring of large YSO samples with a wide variety of professional and amateur telescopes. We presen…
Variability in IC5070: two young stars with deep recurring eclipses
D. Froebrich, A. Scholz, J. Campbell-White +7
We present two low-mass YSOs in IC5070 (V1490Cyg, V1706Cyg) with deep recurring eclipses.
A survey for variable young stars with small telescopes: First results from HOYS-CAPS
D. Froebrich, J. Campbell-White, A. Scholz +15
Variability in Young Stellar Objects (YSOs) is one of their primary characteristics. Long-term, multi-filter, high-cadence monitoring of large YSO samples is the key to understand…
YSO jets in the Galactic Plane from UWISH2: IV - Jets and outflows in Cygnus-X
S. V. Makin, D. Froebrich
We have performed an unbiased search for outflows from young stars in Cygnus-X using 42 deg of data from the UKIRT Widefield Infrared Survey for H (UWISH2 survey), to ident…
YSO jets in the Galactic Plane from UWISH2: III - Jets and Outflows in Cassiopeia and Auriga
D. Froebrich, S. V. Makin
We present the analysis of 35.5 square degrees of images in the 1-0S(1) line of H2 from the UK Widefield Infrared Survey for H2 (UWISH2) towards Cassiopeia and Auriga. We have iden…
The UWISH2 extended H2 source catalogue
D. Froebrich, S. V. Makin, C. J. Davis +9
We present the extended source catalogue for the UKIRT Widefield Infrared Survey for H2 (UWISH2). The survey is unbiased along the inner Galactic Plane from l \approx 357deg to l \…