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Join “AGN Coffee” Hosted by the AGN SIG

Thursday March 5th, 2026, 1:00 ‑ 2:00pm ET

☕ AGN Coffee - Monthly, informal, and for early-career astronomers ☕

Please join our online discussion space aimed at undergraduate students, graduate students, post-bacs, and postdocs who want a low-pressure way to talk about recent AGN papers and ideas.

📅 First Thursday of every month
🕐 1-2 pm ET
📍 Online (details via Discord: https://discord.com/invite/AuVRMHrv4)

The goal is simple: an informal, community-driven conversation about current AGN research and developments, no talks, no slides, just discussion.

👉 Senior AGN folks: if you work with students or early-career researchers, we’d really appreciate you sharing this with them or encouraging them to join.

This activity is organized by the AGN Science Interest Group (AGN SIG):
https://science.nasa.gov/astrophysics/programs/cosmic-origins/community/agn-sig/

For further questions or access issues please contact the AGN SIG Chair, Erin Hicks (ekhicks@alaska.edu) or the series organizer Anika Goel (anikgoel@iu.edu)

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Angled from the upper left corner to the lower right corner is a cone-shaped orange-red cloud known as Herbig-Haro 49/50. This feature takes up about three-fourths of the length of this angle. The upper left end of this feature has a translucent, rounded end. The conical feature widens slightly from the rounded end at the upper right down to the lower right. Along the cone there are additional rounded edges, like edges of a wave, and intricate foamy-like details, as well as a clearer view of the black background of space. In the upper left, overlapping with the rounded end of Herbig-Haro 49/50, is a background spiral galaxy with a concentrated blue center that fades outward to blend with red spiral arms. The background of space is speckled with some white stars and smaller, more numerous, fainter white galaxies throughout.