| Name | 8711 |
| Title | C/O abundance ratios across WCL planetary nebulae with strong PAH and crystalline silicate emission |
| URL | https://hst.esac.esa.int/ehst/#/pages/search;proposal=8711;TAPCLIENT=DOI |
| DOI | https://doi.org/10.5270/esa-39i9k7b |
| 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=8711&mission=hst |
| Publication | A close look into the carbon disk at the core of the planetary nebula CPD-56°8032, Chesneau, O.,Collioud, A.,De Marco, O., Astronomy and Astrophysics, 455, 2006-09-01 00:00:00, 2006A&A...455.1009C||Discovery of an Edge-on Dust Disk around the [WC10] Central Star CPD -56°8032, De Marco, Orsola,Barlow, M. J.,Cohen, M., The Astrophysical Journal, 574, 2002-07-01 00:00:00, 2002ApJ...574L..83D||The cooling-down central star of the planetary nebula SwSt 1: a late thermal pulse in a massive post-AGB star?, Hajduk, Marcin,Todt, Helge,Hamann, Wolf-Rainer, Monthly Notices of the Royal Astronomical Society, 498, 2020-08-01 00:00:00, 2020MNRAS.498.1205H||Wolf-Rayet Central Stars and the Binary Evolution Channel, De Marco, O.,Sandquist, E. L.,Mac Low, M.-M., Revista Mexicana de Astronomia y Astrofisica Conference Series, 18, 2003-09-01 00:00:00, 2003RMxAC..18...24D |
| Instrument | STIS/CCD, STIS/NUV-MAMA |
| Temporal Coverage | 2000-09-27T04:18:05Z/2001-04-11T10:24:09Z |
| 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 | 2007-01-23T14:58:28Z |
| Publisher And Registrant | European Space Agency |
| Credit Guidelines | European Space Agency, 2007, C/O Abundance Ratios Across Wcl Planetary Nebulae With Strong Pah And Crystalline Silicate Emission, 1.0, European Space Agency, https://doi.org/10.5270/esa-39i9k7b |