The lonely RX J1856.5-3754 [
http://www.eso.org/…] was formed from the collapsed core of an exploding star. At a distance of 180 light-years it is the closest known [
http://arXiv.org/ab…] neutron star. More massive than the Sun but only 20 kilometers across, this tiny stellar juggernaut plows through the hydrogen gas and dust clouds of interstellar space at about 200 kilometers per second. The surface of the neutron star [
http://www.astro.um…] is fantastically hot, around 700,000 degrees Celsius, making it detectable with orbiting x-ray telescopes. But optical astronomers were recently surprised to discover that RX J1856.5-3754 is also surrounded by a cone-shaped nebula. Indicated in this deep image from the European Southern Observatory's Kueyen telescope [
http://antwrp.gsfc.…], the nebula glows in the red light of ionized hydrogen atoms recombining with [
http://csep10.phys.…absorption.html ] electrons. Its cone shape is analogous [
http://antwrp.gsfc.…] to the bow wave of a ship plowing through water. A faint blue dot near the tip of the cone is the neutron star itself. The nebula appears to have formed very near the surface [
http://antwrp.gsfc.…] of the neutron star and astronomers are trying to determine if the observed densities and temperatures can indeed explain the nebula's appearance.
Explanation
The lonely RX J1856.5-3754 [
http://www.eso.org/…] was formed from the collapsed core of an exploding star. At a distance of 180 light-years it is the closest known [
http://arXiv.org/ab…] neutron star. More massive than the Sun but only 20 kilometers across, this tiny stellar juggernaut plows through the hydrogen gas and dust clouds of interstellar space at about 200 kilometers per second. The surface of the neutron star [
http://www.astro.um…] is fantastically hot, around 700,000 degrees Celsius, making it detectable with orbiting x-ray telescopes. But optical astronomers were recently surprised to discover that RX J1856.5-3754 is also surrounded by a cone-shaped nebula. Indicated in this deep image from the European Southern Observatory's Kueyen telescope [
http://antwrp.gsfc.…], the nebula glows in the red light of ionized hydrogen atoms recombining with [
http://csep10.phys.…absorption.html ] electrons. Its cone shape is analogous [
http://antwrp.gsfc.…] to the bow wave of a ship plowing through water. A faint blue dot near the tip of the cone is the neutron star itself. The nebula appears to have formed very near the surface [
http://antwrp.gsfc.…] of the neutron star and astronomers are trying to determine if the observed densities and temperatures can indeed explain the nebula's appearance.
Explanation
