Results 131 to 140 of about 30,917 (231)
The Panchromatic Hubble Andromeda Southern Treasury (PHAST) is a large 195-orbit Hubble Space Telescope program imaging ∼0.45 deg ^2 of the southern half of M31's star-forming disk at optical and near-ultraviolet (NUV) wavelengths.
Zhuo Chen +27 more
doaj +1 more source
Massive stars dying alone: The extremely remote environment of SN 2009ip
We present late-time HST images of the site of supernova (SN) 2009ip taken almost 3 yr after its bright 2012 luminosity peak. SN 2009ip is now slightly fainter in broad filters than the progenitor candidate detected by HST in 1999.
Andrews, Jennifer E. +2 more
core +1 more source
Supernova Remnants and the Interstellar Medium of M83: Imaging & Photometry with WFC3 on HST
We present Wide Field Camera 3 images taken with the Hubble Space Telescope within a single field in the southern grand design star-forming galaxy M83. Based on their size, morphology and photometry in continuum-subtracted H$ $, [\SII], H$ $, [\OIII] and [\OII] filters, we have identified 60 supernova remnant candidates, as well as a handful of young
Dopita, Michael A. +25 more
openaire +2 more sources
Characterizing the Star Cluster Populations in Stephan’s Quintet Using HST and JWST Observations
Stephan’s Quintet (SQ) is a local compact galaxy group system that exhibits significant star formation activity. A history of tidal interactions between its four member galaxies and a recent collision between an intruder galaxy and the original group are
P. Aromal +16 more
doaj +1 more source
The effects of dust on the optical and infrared evolution of SN 2004et
We present an analysis of multi-epoch observations of the Type II-P supernova SN 2004et. New and archival optical spectra of SN 2004et are used to study the evolution of the Halpha and [O I] 6300A line profiles between days 259 and 646.
Andrews +82 more
core +2 more sources
Deep HST-WFPC2 photometry of NGC 288. I. Binary Systems and Blue Stragglers
We present the first results of a deep WFPC2 photometric survey of the loose galactic globular cluster NGC 288. The fraction of binary systems is estimated from the color distribution of objects near the Main Sequence (MS) with a method analogous to that introduced by Rubenstein & Bailyn(1997).
Bellazzini, M. +4 more
openaire +2 more sources
Cosmicflows-2 is a compilation of distances and peculiar velocities for over 8000 galaxies. Numerically the largest contributions come from the luminosity-linewidth correlation for spirals, the TFR, and the related Fundamental Plane relation for E/S0 ...
Courtois, Helene M. +13 more
core +3 more sources
Constraints on thick disc and halo parameters from HST photometry of field stars in the Galaxy [PDF]
L. O. Kerber +2 more
openalex +2 more sources
Exploring the Diversity of Faint Satellites in the M81 Group
In the last decade, we have been able to probe further down the galaxy luminosity function than ever before and expand into the regime of ultra-faint dwarfs (UFDs), which are some of the best probes we have of small-scale cosmology and galaxy formation ...
Katya Gozman +11 more
doaj +1 more source
The Faint Satellite System of NGC 253: Insights into Low-density Environments and No Satellite Plane
We have conducted a systematic search around the Milky Way (MW) analog NGC 253 ( D = 3.5 Mpc), as a part of the Panoramic Imaging Survey of Centaurus and Sculptor (PISCeS)—a Magellan+Megacam survey to identify dwarfs and other substructures in resolved ...
Burçin Mutlu-Pakdil +14 more
doaj +1 more source

