DIISC-III. Signatures of Stellar Disk Growth in Nearby Galaxies
DIISC-II: Unveiling the Connections between Star Formation and Interstellar Medium in the Extended Ultraviolet Disk of NGC 3344
DIISC-I: The Discovery of Kinematically Anomalous H I Clouds in M 100
DIISC-IV. DIISCovery of Anomalously Low Metallicity H II Regions in NGC 99: Indirect Evidence of Gas Inflows
DIISC-VI (COS-DIISC): Ultraviolet Metal Absorption Relative to the H I Disk of Galaxies
Evidence for a Rotational Component in the Circumgalactic Medium of Nearby Galaxies
Probing Large Galaxy Halos at Z ~ 0 with Automated Lya-absorption Matching
Probing the physicochemical properties of the Leo Ring and the Leo I group
Reporting a deficit of intrinsic N V absorbers in core-dominated radio-loud quasars
Signatures of gas flows - I. Connecting the kinematics of the H I circumgalactic medium to galaxy rotation
Unveiling the complex circumgalactic medium: a comparative study of merging and non-interacting galaxy groups
Instrument
COS, COS/FUV, COS/NUV
Temporal Coverage
2015-11-23T17:55:25Z/2016-11-04T02:55:28Z
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.
European Space Agency, Borthakur, 2016, 'How are HI Disks Fed? Probing Condensation at the Disk-Halo Interface', 1.0, European Space Agency, https://doi.org/10.5270/esa-xqk9tac
Rights
Data hosted in the ESA Space Science Archives are distributed under the CC BY-NC 3.0 IGO license.