Research output per year
Research output per year
Description
North-PHASE (Periodicity, Hot spots, Accretion Stability and Early evolution in young stellar clusters in the Northern Hemisphere) is a project led by the University of Dundee (UK) that "uses time to map space" to unveil the star-disk connection of young stars during the epochs of planet formation. The physical scales in the inner planet-forming disk and star are too small to be addressed by direct imaging, but time-resolved, multi-band photometric variability with broad- and narrow-band filters allows us to explore accretion, stellar spots and occultations by the innermost disk. Over 5 years, we can study how these change in timescales similar to inner planet orbits for thousands of young stars in clusters.
Data are available as virtual observatory tables (VO) that can be downloaded or queried via ADQL.
Copyright © 2024 North Phase Team. All Rights Reserved.
Data are available as virtual observatory tables (VO) that can be downloaded or queried via ADQL.
Copyright © 2024 North Phase Team. All Rights Reserved.
| Date made available | Jul 2024 |
|---|---|
| Publisher | Center for Cosmos Physics Studies of Aragon |
Research output
- 1 Article
-
North-PHASE: studying periodicity, hot spots, accretion stability, and early evolution in young stars in the Northern hemisphere
Sicilia Aguilar, A. (Lead / Corresponding author), Kahar, R. S., Pelayo-Baldárrago, M. E., Roccatagliata, V., Froebrich, D., Galindo-Guil, F. J., Campbell-White, J., Kim, J. S., Mendigutía, I., Schlueter, L., Teixeira, P. S., Matsumura, S., Fang, M., Scholz, A., Ábrahám, P., Frasca, A., Garufi, A., Herbert, C., Kospal, A. & Manara, C. F., Aug 2024, In: Monthly Notices of the Royal Astronomical Society. 532, 2, p. 2108-2132 25 p.Research output: Contribution to journal › Article › peer-review
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