SN 2013fs is a supernova, located in the spiral galaxy NGC 7610, discovered by the Intermediate Palomar Transient Factory sky survey at Palomar Observatory in October 2013 (and originally named iPTF 13dqy). It was discovered approximately three hours from explosion (first light) and was observed in ultraviolet and X-ray wavelengths, among others, within several hours. Optical spectra were obtained beginning at six hours from explosion, making these the earliest such detailed observations ever made of a supernova.
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| - SN 2013fs (es)
- SN 2013fs (en)
- SN 2013fs (zh)
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| - SN 2013fs是一顆在螺旋星系NGC 7610內發現的超新星。該超新星由帕洛马山天文台的帕洛馬瞬變工廠發現於2013年10月，當時命名為iPTF 13dqy。天文學家在SN 2013fs爆炸後大約3小時觀測到它，並在之後數小時內在紫外線與X射線波段觀測到。天文學家於SN 2013fs爆炸後6小時觀測到它的可見光光譜，因此是至今最迅速獲得如此觀測細節結果的超新星。 (zh)
- SN 2013fs es una supernova, ubicada en la galaxia espiral NGC 7610, descubierta por la Fábrica Transitoria de Palomar en el Observatorio Palomar en octubre de 2013 (y originalmente llamado iPTF 13dqy). Se descubrió aproximadamente 3 horas desde la explosión y se observó en rayos ultravioleta y rayos X, entre otras, durante varias horas. Los espectros ópticos se obtuvieron a partir de las 6 horas de la explosión, haciendo estas las observaciones más detalladas que se hayan hecho de una supernova en tan poco tiempo. (es)
- SN 2013fs is a supernova, located in the spiral galaxy NGC 7610, discovered by the Intermediate Palomar Transient Factory sky survey at Palomar Observatory in October 2013 (and originally named iPTF 13dqy). It was discovered approximately three hours from explosion (first light) and was observed in ultraviolet and X-ray wavelengths, among others, within several hours. Optical spectra were obtained beginning at six hours from explosion, making these the earliest such detailed observations ever made of a supernova. (en)
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| - Earliest detailed observations of a supernova ever made. (en)
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| - SN 2013fs es una supernova, ubicada en la galaxia espiral NGC 7610, descubierta por la Fábrica Transitoria de Palomar en el Observatorio Palomar en octubre de 2013 (y originalmente llamado iPTF 13dqy). Se descubrió aproximadamente 3 horas desde la explosión y se observó en rayos ultravioleta y rayos X, entre otras, durante varias horas. Los espectros ópticos se obtuvieron a partir de las 6 horas de la explosión, haciendo estas las observaciones más detalladas que se hayan hecho de una supernova en tan poco tiempo. La estrella que produjo SN 2013fs fue una supergigante roja, probablemente alrededor de 10 veces la masa de nuestro Sol y no era más de unos pocos millones de años más viejo cuando explotó. La estrella estaba rodeada por una capa relativamente densa de gas arrojado por la estrella dentro antes de que explotara. La radiación emitida por la explosión de la supernova iluminó su cáscara, que tenía una masa de aproximadamente una milésima parte de nuestro sol, y su franja exterior era aproximadamente 5 veces la distancia de Neptuno de nuestro sol. (es)
- SN 2013fs is a supernova, located in the spiral galaxy NGC 7610, discovered by the Intermediate Palomar Transient Factory sky survey at Palomar Observatory in October 2013 (and originally named iPTF 13dqy). It was discovered approximately three hours from explosion (first light) and was observed in ultraviolet and X-ray wavelengths, among others, within several hours. Optical spectra were obtained beginning at six hours from explosion, making these the earliest such detailed observations ever made of a supernova. The star that produced SN 2013fs was a red supergiant with a mass 10 times the mass of the Sun, an effective temperature of 3,500 K, a radius 607 times the size of the Sun, and no more than a few million years old when it exploded. The star was surrounded by a relatively dense shell of gas shed by the star within the year before it exploded. Radiation emitted by the supernova explosion illuminated this shell, which had a mass of approximately one-thousandth the mass of the Sun, and its outer fringe was about five times the distance of Neptune from the Sun. (en)
- SN 2013fs是一顆在螺旋星系NGC 7610內發現的超新星。該超新星由帕洛马山天文台的帕洛馬瞬變工廠發現於2013年10月，當時命名為iPTF 13dqy。天文學家在SN 2013fs爆炸後大約3小時觀測到它，並在之後數小時內在紫外線與X射線波段觀測到。天文學家於SN 2013fs爆炸後6小時觀測到它的可見光光譜，因此是至今最迅速獲得如此觀測細節結果的超新星。 (zh)
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