Revealing a Spiral-Shaped Molecular Cloud in Our Galaxy: Cloud Fragmentation Under Rotation and Gravity

Astronomy and Astrophysics - France
doi 10.1051/0004-6361/201628251
Full Text
Abstract

Available in full text

Date
Authors
Publisher

EDP Sciences

Related search

Cloud-Cloud Collisions and Fragmentation

Symposium - International Astronomical Union
1991English

Cloud-Cloud Collisions and Fragmentation

Symposium - International Astronomical Union
1991English

Dense Core Structure and Fragmentation in the Rho Ophiuchi Molecular Cloud

Symposium - International Astronomical Union
1991English

Dense Core Structure and Fragmentation in the Rho Ophiuchi Molecular Cloud

Symposium - International Astronomical Union
1991English

5.20. Molecular Cloud Properties in the Barred Galaxy NGC 7479

Symposium - International Astronomical Union
1998English

Under a Cloud

Nature
Multidisciplinary
1990English

Molecular Cloud Cores and Protostars: Offsprings of Gravity and Cosmic Magnetism

Symposium - International Astronomical Union
1990English

Signatures of Galaxy-Cluster Interactions: Spiral Galaxy Rotation Curve Asymmetry, Shape, and Extent

Astronomical Journal
AstrophysicsAstronomyPlanetary ScienceSpace
2001English

Rotation Curve of Our Galaxy and Field Galaxies

Symposium - International Astronomical Union
2004English

Amanote Research

Note-taking for researchers

Follow Amanote

© 2026 Amaplex Software S.P.R.L. All rights reserved.

Privacy PolicyRefund Policy