Simeis 147 (Spaghetti Nebula)
Simeis 147, also known as the Spaghetti Nebula (SH2-240), is a supernova remnant in the Milky Way straddling the border between the constellations Auriga and Taurus. Discovered in 1952 at the Crimean Astrophysical Observatory using a 25-inch Schmidt-Cassegrain telescope, it is difficult to observe due to its extremely low brightness. It is believed that after its stellar explosion a rapidly spinning neutron star known as pulsar PSR J0538+2817 was left behind in the nebula core, emitting a strong radio signal. (4 Panel Mosaic, Explore Scientific ED80, ZWO ASI2600MM, ASIAIR, EAF, EFW, AM5, Antlia SHO 3nm, Astropixelprocessor, Pixinsight, Photoshop).
Simeis 147 (Spaghetti Nebula)
Simeis 147, also known as the Spaghetti Nebula (SH2-240), is a supernova remnant in the Milky Way straddling the border between the constellations Auriga and Taurus. Discovered in 1952 at the Crimean Astrophysical Observatory using a 25-inch Schmidt-Cassegrain telescope, it is difficult to observe due to its extremely low brightness. It is believed that after its stellar explosion a rapidly spinning neutron star known as pulsar PSR J0538+2817 was left behind in the nebula core, emitting a strong radio signal. (4 Panel Mosaic, Explore Scientific ED80, ZWO ASI2600MM, ASIAIR, EAF, EFW, AM5, Antlia SHO 3nm, Astropixelprocessor, Pixinsight, Photoshop).