| Name | 10852 |
| Title | Coronagraphic Polarimetry with NICMOS: Dust grain evolution in T Tauri stars |
| URL | https://hst.esac.esa.int/ehst/#/pages/search;proposal=10852;TAPCLIENT=DOI |
| DOI | https://doi.org/10.5270/esa-hpwcjls |
| Author | European Space Agency |
| Description | This is a scientific proposal for HST mission. For specific information please visit https:\\archive.stsci.edu\proposal_search.php?id=10852&mission=hst |
| Publication | A Spectroscopic Census of the M82 Stellar Cluster Population, Konstantopoulos, I. S.,Bastian, N.,Smith, L. J., The Astrophysical Journal, 701, 2009-08-01 00:00:00, 2009ApJ...701.1015K||Investigating Circumstellar Disk Geometry and Dust Properties with Coronagraphic Polarimetry, Perrin, Marshall D.,Duchene, Gaspard,Graham, James R., Exoplanets and Disks: Their Formation and Diversity, 1158, 2009-08-01 00:00:00, 2009AIPC.1158...17P||Spiral Arms in Disks: Planets or Gravitational Instability?, Dong, Ruobing,Najita, Joan R.,Brittain, Sean D., The Astrophysical Journal, 862, 2018-08-01 00:00:00, 2018ApJ...862..103D||The Case of AB Aurigae's Disk in Polarized Light: Is there Truly a Gap?, Perrin, Marshall D.,Schneider, Glenn,Duchene, Gaspard, The Astrophysical Journal, 707, 2009-12-01 00:00:00, 2009ApJ...707L.132P |
| Instrument | NICMOS/NIC2 |
| Temporal Coverage | 2006-09-15T22:38:42Z/2008-06-08T13:22:09Z |
| Version | 1.0 |
| Mission Description | Launched in 1990, the NASA/ESA Hubble Space Telescope remains the premier UV and visible light telescope in orbit. With well over 1.6 million observations from 10 different scientific instruments, the ESA Hubble Science Archive is a treasure trove of astronomical data to be exploited. |
| Creator Contact | https://support.cosmos.esa.int/esdc/index.php?/Tickets/Submit |
| Date Published | 2009-06-09T15:41:21Z |
| Publisher And Registrant | European Space Agency |
| Credit Guidelines | European Space Agency, 2009, Coronagraphic Polarimetry With Nicmos: Dust Grain Evolution In T Tauri Stars, 1.0, European Space Agency, https://doi.org/10.5270/esa-hpwcjls |