You are here

Identifying Green Fuzzy Emission in the Milky Way

Content has no owner

Figure 1. Spectra of three knots of “Green Fuzzy” emission around the G19.88-0.53 MYSO obtained with NIRI on Gemini North. The shaded area marks the passband of the Spitzer filter and includes the wavelength of the molecular hydrogen transition labeled S(9). This emission line is responsible for the enhanced emission in the Spitzer 4.5 micron band and causes the knots to appear “green.” Additional H2 lines detected in the NIRI spectra are denoted with vertical dashed lines.

Figure 2: Spitzer Space Telescope composite 3-color image (background) showing the Gemini NIRI spectral slit location encompassing the MYSO and three knots of green fuzzy emission in G19.88-0.53.

Using the Gemini Near-Infrared Imager and spectrometer (NIRI) on the Gemini North telescope, James De Buizer and William Vacca (SOFIA-USRA) obtained spectra that, for the first time, directly identify the origin of “green fuzzy” emission.

The Spitzer Space Telescope survey of the central plane of the Milky Way Galaxy revealed an unusual feature of some massive star forming regions in the galaxy: areas of extended emission that appear to have enhanced flux at 4.5 microns (which is usually assigned the color green when constructing three-color images from Spitzer data). These so-called “green fuzzies” (or “extended green objects”) were previously associated with massive young stellar objects (MYSOs) in star forming regions, but the exact origin of the emission could not be determined from the images alone.

In one source, known as G19.88-053, the new NIRI data revealed that the enhanced 4.5 micron emission arises from a prominent molecular hydrogen emission line in its spectrum (Figures 1 and 2). The H2 is concentrated in compact knots that are associated with an outflow around the central MYSO. Shocks heat the molecular gas to temperatures of ~2600 K.

However, another “green fuzzy,” associated with a different star-forming region, did not show any emission lines in its NIRI spectrum. The central MYSO of G49.27-0.34 is deeply embedded in surrounding gas and dust, as deep CO absorption in the spectrum indicates. The dust alters the emergent spectrum of both the central source and the surrounding gas and dust, suppressing emission at shorter and longer wavelengths corresponding to blue and red in the false-color Spitzer images (around 3.6 and 8.0 microns), and resulting in the “green” appearance.

The complete results will appear in The Astronomical Journal, and a preprint is currently available

News Archive Filter

The GEMMA Podcast

A podcast about Gemini Observatory and its role in the Era of Multi-Messenger Astronomy. Featuring news related to multi-messenger astronomy (MMA), time-domain astronomy (TDA), our visiting instrument program, and more through interviews with astronomers, engineers, and staff both here at Gemini (North and South) and abroad.

Listen Now