HUBBLE SPACE TELESCOPE MEASURES OF MASS ACCRETION RATES IN THE ORION NEBULA CLUSTER
The present observational understanding of the evolution of the mass accretion rates ([dot over M][subscript acc]) in pre-main-sequence stars is limited by the lack of accurate measurements of [dot over M][subscript acc] over homogeneous and large statistical samples of young stars. Such observation...
Main Authors: | Manara, C. F., Robberto, M., Da Rio, N., Lodato, G., Hillenbrand, L. A., Soderblom, D. R., Stassun, Keivan |
---|---|
Other Authors: | Massachusetts Institute of Technology. Department of Physics |
Format: | Article |
Language: | en_US |
Published: |
IOP Publishing
2015
|
Online Access: | http://hdl.handle.net/1721.1/95503 |
Similar Items
-
THE INITIAL MASS FUNCTION OF THE ORION NEBULA CLUSTER ACROSS THE H-BURNING LIMIT
by: Da Rio, N., et al.
Published: (2015) -
YSOVAR: SIX PRE-MAIN-SEQUENCE ECLIPSING BINARIES IN THE ORION NEBULA CLUSTER
by: Morales-Calderon, M., et al.
Published: (2015) -
Hubble Space Telescope search for the transit of the Earth-mass exoplanet Centauri B b
by: Demory, B.-O., et al.
Published: (2017) -
Stellar occultation studies of Saturn's rings with the Hubble Space Telescope
by: Bosh, Amanda Sachie
Published: (2007) -
HUBBLE SPACE TELESCOPE NEAR-ULTRAVIOLET SPECTROSCOPY OF BRIGHT CEMP-s STARS
by: Placco, Vinicius M., et al.
Published: (2016)