This work has been extended and updated in 2025:
- “The Milky Way as Seen by Classical Cepheids I: Distances Based on Mid-infrared Photometry”-> arxiv.org/abs/2406.09113
- “The Milky Way as Seen by Classical Cepheids II: Spiral Structure”-> arxiv.org/abs/2406.09127
This work has been extended and updated in 2025:
- “The Milky Way as Seen by Classical Cepheids I: Distances Based on Mid-infrared Photometry”-> arxiv.org/abs/2406.09113
- “The Milky Way as Seen by Classical Cepheids II: Spiral Structure”-> arxiv.org/abs/2406.09127
In 2019, a Warsaw research team presented the first 3D map of the Milky Way in the journal Science.
The map is based on direct distances to thousands of Cepheids.
A pioneering achievement, still widely cited. 🔭🧪⚛️
#galactic #astronomy #universe
In 2019, a Warsaw research team presented the first 3D map of the Milky Way in the journal Science.
The map is based on direct distances to thousands of Cepheids.
A pioneering achievement, still widely cited. 🔭🧪⚛️
#galactic #astronomy #universe
At a distance of 6,000 light-years, the Cepheid variable star was observed by Hubble and is one of the biggest and brightest known Cepheids in the Milky Way galaxy.
Processed by @thocarp.bsky.social
www.flickr.com/photos/19746...
🔭 🧪
At a distance of 6,000 light-years, the Cepheid variable star was observed by Hubble and is one of the biggest and brightest known Cepheids in the Milky Way galaxy.
Processed by @thocarp.bsky.social
www.flickr.com/photos/19746...
🔭 🧪
Bonus — it has helped us nail down the cosmic distance ladder using Cepheids and Type Ia supernovae.
Definitely worth your time — go read the article! 🧪📖
badastronomy.beehiiv.com/p/happy-sols...
🔭 🧪
Bonus — it has helped us nail down the cosmic distance ladder using Cepheids and Type Ia supernovae.
Definitely worth your time — go read the article! 🧪📖
Data: NGC-3370, released 2025-05-24
NASA, STSci/ #JWST, NIRCam /RGB: 277, 150, 090
Data: NGC-3370, released 2025-05-24
NASA, STSci/ #JWST, NIRCam /RGB: 277, 150, 090
minouette.etsy.com/listing/4518...
minouette.etsy.com/listing/4518...
target: NGC-2525, released: 2025-11-17
NASA, ESA, CSA, STSci/ #JWST NIRCam 277, 150
target: NGC-2525, released: 2025-11-17
NASA, ESA, CSA, STSci/ #JWST NIRCam 277, 150
Of a woman who watches Cepheids quaver
among lightbursting mangroves.
Of a woman who watches Cepheids quaver
among lightbursting mangroves.
Scrutinizing the Dirtiest Cepheids, a Test of the Hubble Tension
TARG: #NGC2525
2024-11-16
PI: Riess, Adam
NIRCAM 277 150 090
yuval-harpaz.github.io/astro/jwst_l...
NASA/ESA/CSA/STScI/j. Roger
Scrutinizing the Dirtiest Cepheids, a Test of the Hubble Tension
TARG: #NGC2525
2024-11-16
PI: Riess, Adam
NIRCAM 277 150 090
yuval-harpaz.github.io/astro/jwst_l...
NASA/ESA/CSA/STScI/j. Roger
Image date: 9 June 1993, 06:00
Credit: NASA/ESA, STScI
Source: ESA/Hubble
Image date: 9 June 1993, 06:00
Credit: NASA/ESA, STScI
Source: ESA/Hubble
#linocut #printmaking #astronomy
#linocut #printmaking #astronomy
Cepheids are relatively young pulsating supergiant stars whose brightness varies according to a very regular pattern with a well-defined period that can range from a few hours to several tens of days.
They are therefore perfect cosmic tracers.
Cepheids are relatively young pulsating supergiant stars whose brightness varies according to a very regular pattern with a well-defined period that can range from a few hours to several tens of days.
They are therefore perfect cosmic tracers.
It is located some ~80 million light years away from us, and it was observed to study Cepheids to improve our cosmological model.
HD: flic.kr/p/2r5F4Wf
It is located some ~80 million light years away from us, and it was observed to study Cepheids to improve our cosmological model.
HD: flic.kr/p/2r5F4Wf
...spiral arms.
A simple simulation of star formation episodes in the arms, taking into account differential rotation (stars and arms rotate at different speeds), reproduces well the overdensities observed today.
It confirms that many Cepheids formed in the arms and then moved away.
...spiral arms.
A simple simulation of star formation episodes in the arms, taking into account differential rotation (stars and arms rotate at different speeds), reproduces well the overdensities observed today.
It confirms that many Cepheids formed in the arms and then moved away.
The team measured 2,431 classical Cepheids, most of them discovered by the OGLE survey.
Infrared period-luminosity relations gave distances accurate to better than 5%.
This is the first map that reaches the outer edge of the disk using individual stars.
The team measured 2,431 classical Cepheids, most of them discovered by the OGLE survey.
Infrared period-luminosity relations gave distances accurate to better than 5%.
This is the first map that reaches the outer edge of the disk using individual stars.
Data: NGC-3447, released 2025-05-23
NASA, STSci/ #JWST, NIRCam / RGB: 356, 277, 150
Data: NGC-3447, released 2025-05-23
NASA, STSci/ #JWST, NIRCam / RGB: 356, 277, 150