Name | 9897 |
Title | Time Scales for Gas Transport, Star Formation, and AGN Fueling in the Born-again Radio Galaxy 3C236 |
URL | https://hst.esac.esa.int/ehst/#/pages/search;proposal=9897;TAPCLIENT=DOI |
DOI | https://doi.org/10.5270/esa-q2354o4 |
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=9897&mission=hst |
Publication | Episodic Star Formation Coupled to Reignition of Radio Activity in 3C 236, Tremblay, Grant R.,O'Dea, Christopher P.,Baum, Stefi A., The Astrophysical Journal, 715, 2010-05-01 00:00:00, 2010ApJ...715..172T||Feedback Regulated Star Formation in Cool Core Clusters of Galaxies, Tremblay, Grant, Ph.D. Thesis, 0, 2011-01-01 00:00:00, 2011PhDT........21T||Fueling the central engine of radio galaxies. II. The footprints of AGN feedback on the ISM of 3C 236, Labiano, A.,GarcĂa-Burillo, S.,Combes, F., Astronomy and Astrophysics, 549, 2013-01-01 00:00:00, 2013A&A...549A..58L||Mapping the neutral atomic hydrogen gas outflow in the restarted radio galaxy 3C 236, Schulz, R.,Morganti, R.,Nyland, K., Astronomy and Astrophysics, 617, 2018-09-01 00:00:00, 2018A&A...617A..38S |
Instrument | ACS, ACS/HRC, ACS/SBC, ACS/WFC, STIS/CCD, STIS/NUV-MAMA |
Temporal Coverage | 2003-10-19T02:40:12Z/2004-01-01T05:14:06Z |
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 | 2005-01-01T05:14:06Z |
Publisher And Registrant | European Space Agency |
Credit Guidelines | European Space Agency, 2005, Time Scales For Gas Transport, Star Formation, And Agn Fueling In The Born-Again Radio Galaxy 3C236, 1.0, European Space Agency, https://doi.org/10.5270/esa-q2354o4 |