| Name | 12885 |
| Title | Kepler's SNR: A Type Ia Supernova from a Single Degenerate System? |
| URL | https://hst.esac.esa.int/ehst/#/pages/search;proposal=12885;TAPCLIENT=DOI |
| DOI | https://doi.org/10.5270/esa-w3s74me |
| 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=12885&mission=hst |
| Publication | An Ejecta Kinematics Study of Kepler's Supernova Remnant with High-resolution Chandra HETG Spectroscopy, Millard, M. J.,Bhalerao, Jayant,Park, Sangwook, The Astrophysical Journal, 893, 2020-04-01 00:00:00, 2020ApJ...893...98M||Carbon, Helium, and Proton Kinetic Temperatures in a Cygnus Loop Shock Wave, Raymond, J. C.,Edgar, Richard J.,Ghavamian, Parviz, The Astrophysical Journal, 805, 2015-06-01 00:00:00, 2015ApJ...805..152R||No Surviving Companion in Kepler's Supernova, Ruiz-Lapuente, Pilar,Damiani, F.,Bedin, L. R., The Astrophysical Journal, 862, 2018-08-01 00:00:00, 2018ApJ...862..124R||Second Epoch Hubble Space Telescope Observations of Kepler's Supernova Remnant: The Proper Motions of Balmer Filaments, Sankrit, Ravi,Raymond, J. C.,Blair, William P., The Astrophysical Journal, 817, 2016-01-01 00:00:00, 2016ApJ...817...36S |
| Instrument | WFC3, WFC3/UVIS |
| Temporal Coverage | 2013-07-01T14:02:12Z/2013-07-03T22:39:39Z |
| 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 | 2014-07-04T04:10:57Z |
| Publisher And Registrant | European Space Agency |
| Credit Guidelines | European Space Agency, 2014, Kepler'S Snr: A Type Ia Supernova From A Single Degenerate System?, 1.0, European Space Agency, https://doi.org/10.5270/esa-w3s74me |