Kilonova y Galaxy anfitriona

Kilonova y Galaxy anfitriona

Un equipo de científicos ha utilizado el telescopio espacial James Webb de la NASA para observar una explosión de rayos gamma excepcionalmente brillante, GRB 230307A y su kilonova asociada. Kilonovas, una explosión producida por una estrella de neutrones que se fusiona con un agujero negro o con otra estrella de neutrones, son extremadamente raros, lo que dificulta observar estos eventos. Las capacidades infrarrojas altamente sensibles de Webb ayudaron a los científicos a identificar la dirección de la casa de las dos estrellas de neutrones que crearon la Kilonova.

Esta imagen del instrumento NIRCAM (cámara cercana de infrarrojo) de Webb resalta el Kilonova de GRB 230307A y su antigua galaxia local entre sus entornos locales de otras galaxias y estrellas en el frente. Las estrellas de los neutrones fueron expulsadas de su galaxia local y viajaron a la distancia de aproximadamente 120,000 años luz, aproximadamente el diámetro de la Vía Láctea, antes de fusionar finalmente varios cientos de millones de años después.

credits

Image

nasa, Esa, CSA, Stsci yw Levan (IMapp, Warw)

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About The Object
Object Name GRB 230307A
Object Description Gamma ray burst from two colliding nuetron stars 
R.A. Position 04:03:26.01
Dec. Position -75:22:42.78
Constellation Mensa
Dimensions Image is approximately 1.3 arcminutes across
About The Data
Data Description The Webb observations include those from program: (A. Levan) 
Instrument NIRCam
Exposure Dates 05 April 2023, 08 May 2023
Filters F115W, F150W, F277W, F356W, F444W
About The Image
Color Info This image is a composite of separate exposures acquired by the James Webb Space Telescope using the NIRCam instrument. Several filters were used to sample wide wavelength ranges. The color results from assigning different hues (colors) to each monochromatic (grayscale) image associated with an individual filter. In this case, the assigned colors are:  Blue: F115W + F150W Green: F277W Red: F356W + F444W
Compass Image Bright galaxies and other light sources in various sizes and shapes are scattered across a black swath of space: small points, hazy elliptical-like smudges with halos, and spiral-shaped blobs. The objects vary in color: white, blue-white, yellow-white, and orange-red. Toward the center right is a blue-white spiral galaxy seen face-on that is larger than the other light sources in the image. The galaxy is labeled “former home galaxy.” Toward the upper left is a small red point, which has a white circle around it and is labeled “GRB 230307A kilonova.”
About The Object
Object Name A name or catalog number that astronomers use to identify an astronomical object.
Object Description The type of astronomical object.
R.A. Position Right ascension – analogous to longitude – is one component of an object's position.
Dec. Position Declination – analogous to latitude – is one component of an object's position.
Constellation One of 88 recognized regions of the celestial sphere in which the object appears.
Distance The physical distance from Earth to the astronomical object. Distances within our solar system are usually measured in Astronomical Units (AU). Distances between stars are usually measured in light-years. Interstellar distances can also be measured in parsecs.
Dimensions The physical size of the object or the apparent angle it subtends on the sky.
About The Data
Data Description
  • Proposal: A description of the observations, their scientific justification, and the links to the data available in the science archive.
  • Science Team: The astronomers who planned the observations and analyzed the data. "PI" refers to the Principal Investigator.
Instrument The science instrument used to produce the data.
Exposure Dates The date(s) that the telescope made its observations and the total exposure time.
Filters The camera filters that were used in the science observations.
About The Image
Image Credit The primary individuals and institutions responsible for the content.
Publication Date The date and time the release content became public.
Color Info A brief description of the methods used to convert telescope data into the color image being presented.
Orientation The rotation of the image on the sky with respect to the north pole of the celestial sphere.