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A science-oriented feed about Galactic astronomy. Part of the Astronomy feeds network. Astronomers can sign up to post here via @bot.astronomy.blue Contains posts from signed up users with #galactic or #galacticastro. Posts here are also included in the main Astronomy feed.

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  • 💙 Liked by 166 users
  • 📅 Updated about 2 months ago
  • ⚙️ Provider feed-all.astronomy.blue

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Astronomy Feeds News
@astronomy.blue
8 months ago
The Astronomy feeds now include 11 (!!!) brand new specific subfeeds! 🔭 The subfeeds try to cover every part of astronomy research with at least one feed. All subfeeds automatically crosspost to the main Astronomy feed, too! Here's a thread with links to all of them ⬇️
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Emily Hunt
@emily.space
1 day ago
Interesting #galactic paper out today that finds that the stellar stream OCSN 49 is likely a disrupted galactic open cluster. ☄️🧪 What destroyed it 100 million years ago? Alexis N. Miller et al have the answers: it probably got torn apart by a massive cloud of gas & dust ⬇️
Evidence for a Catastrophically Disrupted Open Cluster

arxiv.org

Evidence for a Catastrophically Disrupted Open Cluster

Of the many discoveries uncovered by the Gaia astrometric mission, some of the most exciting are related to nearby dispersed stellar structures. We analyze one such structure in the Milky Way disk, OC...

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@drnereide.bsky.social
2 days ago
3/ In a space only 1000 light-years across, there are numerous and complex interactions due to: expanding supernova remnants, hot winds from newly formed stars, unusually strong and colliding magnetic fields, and Sagittarius A*, our Galaxy's supermassive black hole. 🔭 🧪 #cosmology #galactic
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@drnereide.bsky.social
2 days ago
2/ and magnetic fields near the Galactic Center. The area depicted is about 1,000 light-years across and 2,000 light-years long. It is in Sagittarius some 26,000 light-years from Earth. This labeled version points out interesting sights to see. 🔭 🧪 #cosmology #galactic
This is the labeled version of the primary image. It points out interesting sights to see.
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@drnereide.bsky.social
2 days ago
🧵 This panoramic image, combining X-rays from Chandra (orange, green, purple) & radio data (gray) from the MeerKAT telescope, provides an unprecedented view above and below the center of the Milky Way, revealing threads of superheated gas ➡️ chandra.si.edu/photo/2021/g... 🔭 🧪 #cosmology #galactic
The image reveal threads of superheated gas and magnetic fields near the center of the Milky Way. It combines X-rays from Chandra and radio data from the MeerKAT telescope. X-rays are orange, green, blue, and purple. Radio is lilac and gray.
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@drnereide.bsky.social
8 days ago
1/2 Happy Earth Day! That pale blue dot in the pic is Earth, our home! The view of Earth from space helps us understand how interconnected we are, reminds us of our fragility and the need to preserve this home for future generations. ➡️ www.esa.int/ESA_Multimed... 🔭 🧪 #EarthDay2025 #galactic
This image from Cassini spacecraft has captured Saturn’s rings and our planet Earth and Moon in the same frame.
The dark side of Saturn, its bright limb, the main rings, the F ring, and the G and E rings are clearly seen; the limb of Saturn and the F ring are overexposed. The E and G rings have been brightened for better visibility.
Earth, 1.44 billion km away in the image, appears as a blue dot at centre right; the Moon can be seen as a fainter protrusion off its right side. The other bright dots nearby are stars.
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@drnereide.bsky.social
8 days ago
The JWST’s Mid-Infrared Instrument (MIRI) captured an unprecedented image of the planetary nebula NGC 1514 (also known as the Crystal Ball Nebula), located about 1,500 ly from Earth in the constellation Taurus. Reference➡️ esawebb.org/news/weic2508/ 🔭 🧪 #JWST #Webb #galactic
This #JWST image shows the planetary nebula NGC 1514 with a tilted hourglass structure. In the center, two stars appear as a single bright point with diffraction rays. The fuzzy orange dust rings form intricate patterns, with a "tight waist" visible at the top left and bottom right. Translucent orange clouds add volume to the nebula, while the pink central region shows sharp holes. A bright blue star, not part of the nebula, stands out at the bottom left.
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International Astronomical Youth Camp
@iayc.bsky.social
8 days ago
Our very own galaxy — here are some amazing photos of the Milky Way taken in El Solitario, Spain back in 2017! IAYC is a perfect place to learn how to observe 🌌 All images were taken by leader Javier Barrios Martí during camp 🔭 #astrophotography #astroedu #astrophotos #galactic #spacephotography
Milky Way over observation area set up on dirt road
Milky Way above mountains in Baños del Montemayor
Milky way over observation area on dirt road, participants in frame
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@drnereide.bsky.social
10 days ago
🧵 This striking image features the Cat's Eye Nebula (officially NGC 6543), one of the most beautiful & studied planetary nebulae, visible in the northern constellation of Draco. ➡️ apod.nasa.gov/apod/ap19050... In a few billion years our Sun will exhaust its nuclear fuel, expanding 🔭 🧪 #galactic
This stunning composite image shows the Cat's Eye Nebula, a cloud of gas ejected from a dying Sun-like star. At its center, a bright, whitish core is surrounded by concentric rings of gas, fading into shades of blue. Complex, symmetrical internal structures, including filaments and arcs, intertwine in a detailed pattern. In the background, a black sky is dotted with distant stars. X-ray lights, in shades of purple, highlight energetic regions scattered throughout the nebula. The image appears as a celestial sculpture, suspended in space. #Hubble #Chandra
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@drnereide.bsky.social
11 days ago
🧵 NGC 6302, also known as the Butterfly Nebula, is a remarkable example of how stars, as they age, can take on some nice shapes sometimes resembling flowers or insects. ➡️ apod.nasa.gov/apod/ap22112... This #Hubble image has been processed to highlight incredible 🔭 🧪 #stellarastro #galactic
#Hubble' s image shows the Butterfly Nebula (NGC 6302), a planetary nebula with a symmetrical structure resembling butterfly wings. In the center, a dense ring of dust obscures the central star. The nebula expands in vivid hues: deep blue (oxygen), bright green (hydrogen), and hot red (nitrogen), creating a bright, layered effect against a black background of space. The gaseous "wings" extend widely, with intricate details and glowing filaments.
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@drnereide.bsky.social
12 days ago
🧵 Here is Earth's rotation realized in an unusual way: using a camera scanning the landscape of Tivoli, Namibia, Bartosz Wojczyński focused on the sky. He created a timelapse spanning 24 h that has a focal point in the sky rather than on the ground. ➡️ apod.nasa.gov/apod/ap20070... 🔭 🧪 #galactic
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@drnereide.bsky.social
14 days ago
🧵 This intriguing NIRCam (Near-Infrared Camera) image from #JWST shows, in incredible detail, a view of remnant supernova Cassiopeia A (Cas A), including the expanding shell of material flapping into the gas shed by the star before its explosion. ➡️ nasa.gov/missions/web... 🔭 🧪 #galactic
The image of Cassiopeia A (Cas A) taken by the #JWST shows a supernova remnant in near-infrared light. The scene is dominated by a bright inner shell with compact clumps in bright shades of pink and orange, representing sulfur, oxygen, argon, and neon. A large, streaked blob, nicknamed Baby Cas A, appears in the lower right corner, visible in lighter shades.
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@drnereide.bsky.social
16 days ago
🧵 This breathtaking 315-million-pixel composite from Hubble shows Chamaeleon Cloud I (Cha I), one of three segments within the Chamaeleon Cloud Complex, a huge star forming region at the surface of the Local Bubble. ➡️ science.nasa.gov/missions/hub... 🔭 🧪 #galactic #Hubble #HST
This Hubble image features a portion of the star-forming region Chamaeleon Cloud Complex, called Cha I. It contains dark, dusty clouds, reflection nebulae lit by bright young blue stars, and bright orange and white knots called Herbig-Haro objects, with jets of hot gas ejected from a protostar at the center of an orange-white cloud below. Bright stars have cross-shaped peaks.
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@drnereide.bsky.social
18 days ago
🧵 The massive star-forming molecular cloud Sagittarius C, located about 200 ly from the SMBH Sagittarius A* at the heart of the Milky Way, despite its abundance of gas and dust, produces fewer stars than expected. Image source➡️ webbtelescope.org/contents/med... 🔭 🧪 #galactic #cosmology
Images from the MeerKAT and JWST telescopes show the star-forming region Sagittarius C, about 200 light-years from Sagittarius A*, the SMBH at the center of the Milky Way. The images include orientation arrows and scale bars for context.

Radio data from MeerKAT reveal large vertical filamentary structures, while Webb captures similar, smaller filaments in a cloud of blue-green hydrogen in the infrared. Colors in the radio data are assigned based on spectral index.
For Webb, colors are created by shifting the infrared spectrum to visible light: shorter infrared wavelengths appear blue, longer ones appear redder.
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@drnereide.bsky.social
18 days ago
🧵 In the past I shared different images of the beautiful Rosette Nebula, but I couldn't resist this fascinating close-up view by Tommy Lease (Denver Astronomical Society). Image source➡️ apod.nasa.gov/apod/ap24020... Technical details➡️ astrobin.com/net448 🔭 🧪 #galactic
The Rosette Nebula, depicted in a close-up astronomical image, resembles a cosmic flower spanning 50 light-years across. The nebula glows with vibrant colors: sulfur emissions create red hues, hydrogen emits green tones, and oxygen contributes blue shades. These colors blend to form an intricate, multi-hued cloud of gas and dust, illuminated by energetic starlight, evoking a delicate, rose-like structure against the dark expanse of space.
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Emily Hunt
@emily.space
19 days ago
It's not a high statistical significance measurement by any means, but I think this is a great pilot study that shows the importance of measuring this for all of the Milky Way's streams! Having multiple measurements would help to constrain the problem a lot more. #galactic 🧪
Galactic Accelerations from the GD-1 Stream Suggest a Tilted Dark Matter Halo

arxiv.org

Galactic Accelerations from the GD-1 Stream Suggest a Tilted Dark Matter Halo

Cold dark matter halos are expected to be triaxial and often tilted relative to the stellar disk. Stellar streams provide a sensitive tracer of the Milky Way's halo shape, though models for the Galact...

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Emily Hunt
@emily.space
19 days ago
There's a very interesting new #galactic paper by Jacob Nibauer & Ana Bonaca on the acceleration of the GD-1 stellar stream around the Milky Way! 🧪 GD-1's orbit is a bit odd: they find a 2σ deviation from a rotationally symmetric dark mater halo! Meaning: our galaxy's dark matter may be a bit flat.
Their fig. 2, showing acceleration predicted by usual models of our galaxy (lines) vs. the model they infer from GD-1's acceleration (shaded region.)
Their figure 5, showing the parameters they infer for the Milky Way's dark matter distribution. it's a bit tilted (dashed cyan lines) compared to the galaxy's assumed total matter density (heatmap).
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Kimberly Emig
@kimager.bsky.social
21 days ago
Radio Recombination lines have now been detected from proplyds! the line emission is mainly coming from an (externally) ionized cloud surface layer that is ~0.01 AU wide, the thickness of the ionization front 😲 great work, Ryan!! public.nrao.edu/news/alma-de... #exoplanets #galactic #astrosci
ALMA Detects First-Ever Hydrogen Recombination Lines From Proplyd Disks in Densely Packed Orion Nebula Cluster - National Radio Astronomy Observatory

public.nrao.edu

ALMA Detects First-Ever Hydrogen Recombination Lines From Proplyd Disks in Densely Packed Orion Nebula Cluster - National Radio Astronomy Observatory

Most stars form in clusters, where hundreds to thousands of stars coevolve in proximal environmental conditions that dictate how...

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@drnereide.bsky.social
24 days ago
2/2 This study, led by UNSW Sydney researchers, focuses on 27 stars with similar ages and compositions to our Sun, but in different evolutionary stages. Let's dig deeper... More at my post ➡️ www.tutto-scienze.org/2025/04/m67-... 🔭 🧪 #galactic #stellarastro #cosmology
M67 Stars Sing The Past And The Future: New Discoveries About The Red Giants

www.tutto-scienze.org

M67 Stars Sing The Past And The Future: New Discoveries About The Red Giants

A recent study explores how the acoustic vibrations of stars in the open cluster M67, located 2,700 ly from Earth in the Milky Way, can reve...

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@drnereide.bsky.social
24 days ago
1/2 A recent study explores how the acoustic vibrations of stars in the open cluster M67, located 2,700 ly from Earth in the Milky Way, can reveal crucial information about their internal structure and evolution. Image credit: Sloan Digital Sky Survey | CC BY 4.0 🔭 🧪 #galactic #stellarastro
This image shows the open star cluster M67. Against a deep black background, typical of space, numerous stars stand out, varying in brightness and size. In the foreground, several bright red stars stand out clearly. These red stars contrast with other smaller, fainter stars, which are white or light gray. The arrangement appears sparse and random, without a clear pattern, reflecting the open nature of the cluster. The intense red of the stars in focus adds a distinctive element to the star field.
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Emily Hunt
@emily.space
26 days ago
These are three known bulk 'moving groups' of stars, but this is the first time (I think) that clusters have been connected to them with orbit integration. They suggest in the paper that resonances between stars and the Milky Way's spiral arms / bar are responsible for these groups. ☄️🧪 #galactic
From moving groups to star formation in the Solar Neighborhood

arxiv.org

From moving groups to star formation in the Solar Neighborhood

Moving groups in the solar neighborhood are ensembles of co-moving stars, likely originating due to forces from spiral arms, the Galactic bar, or external perturbations. Their co-movement with young c...

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Emily Hunt
@emily.space
26 days ago
An interesting #galactic paper by Cameren Swiggum (@mac0598.bsky.social) et al. came out today! ☄️🧪 Extending previous work that showed most young star clusters near to the Sun came from just three regions, Cameren shows that actually *all* nearby clusters come from just three regions!
Backwards orbital integration of star clusters near the Sun in their work. Notice how all the grey dots originate in three areas. (Their Fig. 1)
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