Dark nebula | |
---|---|
Observation data: J2000 epoch | |
Right ascension | 20h 39.5m [1] |
Declination | +68° 00.7′[1] |
Distance | 1,400 ly (440[1] pc) |
Constellation | Cepheus |
L 1157 is a dark nebula in the constellation Cepheus. It was catalogued in 1962 by U.S. astronomer Beverly T. Lynds in her Catalogue of Dark Nebulae, becoming the 1157th entry in the table; hence the designation.[2] The cloud contains an estimated 3,900 Solar masses of material.[1] It includes protostars that are ejecting material in bipolar outflows, forming bow shocks in the surrounding ambient gas. Formamide and HCNO have been detected in these shocked regions, among other compounds.[3]