Tag Archive for 'Class 0 protostar'

This Webb image shows part of Lynds 483. Image credit: NASA / ESA / CSA / STScI.

Webb Captures Fantastic Detail of Lynds 483

Mar 7, 2025 by Enrico de Lazaro

Two young protostars are responsible for the shimmering ejections of gas and dust that gleam in orange, blue, and purple in this color image of a portion...

L1527, shown in this image from Webb’s MIRI instrument, is a molecular cloud that harbors the IRAS 04368+2557 protostar. The more diffuse blue light and the filamentary structures in the image come from organic compounds known as polycyclic aromatic hydrocarbons (PAHs), while the red at the center of this image is an energized, thick layer of gases and dust that surrounds the protostar. The region in between, which shows up in white, is a mixture of PAHs, ionized gas, and other molecules. Image credit: NASA / ESA / CSA / STScI.

Webb Sees Hourglass-Shaped Molecular Cloud around Protostar

Jul 3, 2024 by News Staff

Astronomers using the MIRI (Mid-Infrared Instrument) camera aboard the NASA/ESA/CSA James Webb Space Telescope have captured a striking new photo of the...

This Webb image shows HH 211, a Herbig-Haro object located 1,000 light-years away in the constellation of Perseus. Image credit: NASA / ESA / CSA / Webb / T. Ray, Dublin Institute for Advanced Studies.

Outflows from Young Protostars are Mostly Molecular, Webb Astronomers Find

Sep 17, 2023 by Natali Anderson

Herbig-Haro (HH) objects are formed when stellar winds or jets of gas spewing from protostars form shock waves colliding with nearby gas and dust at high...