Matches in SemOpenAlex for { <https://semopenalex.org/work/W3195222562> ?p ?o ?g. }
- W3195222562 endingPage "75" @default.
- W3195222562 startingPage "75" @default.
- W3195222562 abstract "We present Hubble Space Telescope (HST/WFC3) ultraviolet and infrared observations of eight fast radio burst (FRB) host galaxies with sub-arcsecond localizations, including the hosts of three known repeating FRBs. We quantify their spatial distributions and locations with respect to their host galaxy light distributions, finding that they occur at moderate host normalized-offsets of 1.4 $r_e$ ([0.6,2.1] $r_e$; 68% interval), occur on fainter regions of their hosts in terms of IR light, but overall trace the radial distribution of IR light in their galaxies. The FRBs in our tested distribution do not clearly trace the distributions of any other transient population with known progenitors, and are statistically distinct from the locations of LGRBs, H-poor SLSNe, SGRBs, and Ca-rich transients. We further find that most FRBs are not in regions of elevated local star formation rate and stellar mass surface densities in comparison to the mean global values of their hosts. We also place upper limits to the IR flux at the FRB positions of $m_{rm IR}gtrsim!24.8-27.6$~AB~mag, constraining both satellite and background galaxies to luminosities well below the host luminosity of FRB121102. We find that 5/8 FRB hosts exhibit clear spiral arm features in IR light, and that the positions of all well-localized FRBs located in such hosts are consistent with their spiral arms, although not on their brightest regions. Our results do not strongly support the primary progenitor channel of FRBs being connected either with the most massive (stripped-envelope) stars, or with events which require kicks and long delay times (neutron star mergers)." @default.
- W3195222562 created "2021-08-30" @default.
- W3195222562 creator A5001038754 @default.
- W3195222562 creator A5003957484 @default.
- W3195222562 creator A5011012118 @default.
- W3195222562 creator A5015506314 @default.
- W3195222562 creator A5016391781 @default.
- W3195222562 creator A5020689615 @default.
- W3195222562 creator A5027003606 @default.
- W3195222562 creator A5027857474 @default.
- W3195222562 creator A5030668506 @default.
- W3195222562 creator A5049474206 @default.
- W3195222562 creator A5052635891 @default.
- W3195222562 creator A5067783689 @default.
- W3195222562 creator A5088713263 @default.
- W3195222562 creator A5090083121 @default.
- W3195222562 creator A5091683850 @default.
- W3195222562 date "2021-08-01" @default.
- W3195222562 modified "2023-10-16" @default.
- W3195222562 title "A High-resolution View of Fast Radio Burst Host Environments" @default.
- W3195222562 cites W1709217086 @default.
- W3195222562 cites W1848183088 @default.
- W3195222562 cites W1871085321 @default.
- W3195222562 cites W2011301426 @default.
- W3195222562 cites W2014586054 @default.
- W3195222562 cites W2023037133 @default.
- W3195222562 cites W2033803356 @default.
- W3195222562 cites W2035879704 @default.
- W3195222562 cites W2036062947 @default.
- W3195222562 cites W2036423640 @default.
- W3195222562 cites W2037953664 @default.
- W3195222562 cites W2076314139 @default.
- W3195222562 cites W2079227246 @default.
- W3195222562 cites W2092745565 @default.
- W3195222562 cites W2116466430 @default.
- W3195222562 cites W2121795427 @default.
- W3195222562 cites W2123267088 @default.
- W3195222562 cites W2126700402 @default.
- W3195222562 cites W2142238829 @default.
- W3195222562 cites W2289905436 @default.
- W3195222562 cites W2318058028 @default.
- W3195222562 cites W2489612612 @default.
- W3195222562 cites W2560131433 @default.
- W3195222562 cites W2563744641 @default.
- W3195222562 cites W2570838639 @default.
- W3195222562 cites W2571196594 @default.
- W3195222562 cites W2611830765 @default.
- W3195222562 cites W2794558609 @default.
- W3195222562 cites W2896617055 @default.
- W3195222562 cites W2896625698 @default.
- W3195222562 cites W2909593478 @default.
- W3195222562 cites W2953474961 @default.
- W3195222562 cites W2955902629 @default.
- W3195222562 cites W2969285583 @default.
- W3195222562 cites W2990545927 @default.
- W3195222562 cites W2997632089 @default.
- W3195222562 cites W3029501268 @default.
- W3195222562 cites W3030369513 @default.
- W3195222562 cites W3030414242 @default.
- W3195222562 cites W3038929563 @default.
- W3195222562 cites W3082509089 @default.
- W3195222562 cites W3091662953 @default.
- W3195222562 cites W3094691047 @default.
- W3195222562 cites W3098188470 @default.
- W3195222562 cites W3099394385 @default.
- W3195222562 cites W3099845258 @default.
- W3195222562 cites W3100175829 @default.
- W3195222562 cites W3100387168 @default.
- W3195222562 cites W3100783907 @default.
- W3195222562 cites W3101338961 @default.
- W3195222562 cites W3101400699 @default.
- W3195222562 cites W3102756447 @default.
- W3195222562 cites W3102811920 @default.
- W3195222562 cites W3103145119 @default.
- W3195222562 cites W3103868583 @default.
- W3195222562 cites W3104127565 @default.
- W3195222562 cites W3104987194 @default.
- W3195222562 cites W3105353888 @default.
- W3195222562 cites W3105483827 @default.
- W3195222562 cites W3105847478 @default.
- W3195222562 cites W3105970064 @default.
- W3195222562 cites W3106307049 @default.
- W3195222562 cites W3106373846 @default.
- W3195222562 cites W3115113846 @default.
- W3195222562 cites W3125445448 @default.
- W3195222562 cites W3131835702 @default.
- W3195222562 cites W3132160370 @default.
- W3195222562 cites W3197486304 @default.
- W3195222562 cites W4292875581 @default.
- W3195222562 doi "https://doi.org/10.3847/1538-4357/abff56" @default.
- W3195222562 hasPublicationYear "2021" @default.
- W3195222562 type Work @default.
- W3195222562 sameAs 3195222562 @default.
- W3195222562 citedByCount "36" @default.
- W3195222562 countsByYear W31952225622021 @default.
- W3195222562 countsByYear W31952225622022 @default.
- W3195222562 countsByYear W31952225622023 @default.
- W3195222562 crossrefType "journal-article" @default.