Maisons of Tomorrow
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Maha Nawaz is the founder of “Maisons of Tomorrow,” a science & technology blog focused on advancing science journalism.
Joined October 2023
Image shows the dust and gas around the double star system GG Tauri-A. Researchers using ALMA have detected gas in the region between two discs in this binary system. This may allow planets to form in the gravitationally perturbed environment of the binary...
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Image shows the dust and gas around the double star system GG Tauri-A. Researchers using ALMA have detected gas in the region between two discs in this binary system. This may allow planets to form in the gravitationally perturbed environment of the binary...
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Image shows the dust and gas around the double star system GG Tauri-A. Researchers using ALMA have detected gas in the region between two discs in this binary system. This may allow planets to form in the gravitationally perturbed environment of the binary...
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Image shows the dust and gas around the double star system GG Tauri-A. Researchers using ALMA have detected gas in the region between two discs in this binary system. This may allow planets to form in the gravitationally perturbed environment of the binary...
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Image shows the dust and gas around the double star system GG Tauri-A. Researchers using ALMA have detected gas in the region between two discs in this binary system. This may allow planets to form in the gravitationally perturbed environment of the binary...
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Image shows the dust and gas around the double star system GG Tauri-A. Researchers using ALMA have detected gas in the region between two discs in this binary system. This may allow planets to form in the gravitationally perturbed environment of the binary...
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Image shows the dust and gas around the double star system GG Tauri-A. Researchers using ALMA have detected gas in the region between two discs in this binary system. This may allow planets to form in the gravitationally perturbed environment of the binary...
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MIRI images show that the most massive YSOs (young stellar objects) gather near H72.97-69.39 & the less massive YSOs are distributed on the outskirts of N79, a process known as mass segregation...
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MIRI images show that the most massive YSOs (young stellar objects) gather near H72.97-69.39 & the less massive YSOs are distributed on the outskirts of N79, a process known as mass segregation...
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MIRI images show that the most massive YSOs (young stellar objects) gather near H72.97-69.39 & the less massive YSOs are distributed on the outskirts of N79, a process known as mass segregation...
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MIRI images show that the most massive YSOs (young stellar objects) gather near H72.97-69.39 & the less massive YSOs are distributed on the outskirts of N79, a process known as mass segregation...
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MIRI images show that the most massive YSOs (young stellar objects) gather near H72.97-69.39 & the less massive YSOs are distributed on the outskirts of N79, a process known as mass segregation...
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MIRI images show that the most massive YSOs (young stellar objects) gather near H72.97-69.39 & the less massive YSOs are distributed on the outskirts of N79, a process known as mass segregation...
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J1649+2635 is the fourth jet-emitting "Spiral Galaxy" discovered. Nearly 800 million light years from Earth with prominent “jets” of subatomic particles propelled outward at nearly the speed of light. The problem is that spiral galaxies aren't supposed to have such large jets?...
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J1649+2635 is the fourth jet-emitting "Spiral Galaxy" discovered. Nearly 800 million light years from Earth with prominent “jets” of subatomic particles propelled outward at nearly the speed of light. The problem is that spiral galaxies aren't supposed to have such large jets?...
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J1649+2635 is the fourth jet-emitting "Spiral Galaxy" discovered. Nearly 800 million light years from Earth with prominent “jets” of subatomic particles propelled outward at nearly the speed of light. The problem is that spiral galaxies aren't supposed to have such large jets?...
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J1649+2635 is the fourth jet-emitting "Spiral Galaxy" discovered. Nearly 800 million light years from Earth with prominent “jets” of subatomic particles propelled outward at nearly the speed of light. The problem is that spiral galaxies aren't supposed to have such large jets?...
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J1649+2635 is the fourth jet-emitting "Spiral Galaxy" discovered. Nearly 800 million light years from Earth with prominent “jets” of subatomic particles propelled outward at nearly the speed of light. The problem is that spiral galaxies aren't supposed to have such large jets?...
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J1649+2635 is the fourth jet-emitting "Spiral Galaxy" discovered. Nearly 800 million light years from Earth with prominent “jets” of subatomic particles propelled outward at nearly the speed of light. The problem is that spiral galaxies aren't supposed to have such large jets?...
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J1649+2635 is the fourth jet-emitting "Spiral Galaxy" discovered. Nearly 800 million light years from Earth with prominent “jets” of subatomic particles propelled outward at nearly the speed of light. The problem is that spiral galaxies aren't supposed to have such large jets?...
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