In SITU FORMATION OF SgrA* STARS VIA DISK FRAGMENTATION: PARENT CLOUD PROPERTIES AND THERMODYNAMICS

Astrophysical Journal - United States
doi 10.1088/0004-637x/749/2/168
Full Text
Abstract

Available in full text

Date
Authors
Publisher

IOP Publishing

Related search

Close-In Giant-Planet Formation via In-Situ Gas Accretion and Their Natal Disk Properties

Astronomy and Astrophysics
AstrophysicsAstronomyPlanetary ScienceSpace
2019English

Cloud-Cloud Collisions and Fragmentation

Symposium - International Astronomical Union
1991English

Cloud-Cloud Collisions and Fragmentation

Symposium - International Astronomical Union
1991English

Comparison of in Situ and Satellite-Derived Cloud Properties During SUCCESS

Geophysical Research Letters
EarthPlanetary SciencesGeophysics
1998English

Theory of Formation of Massive Stars via Accretion

Symposium - International Astronomical Union
2004English

Disk Formation and Structure

EPJ Web of Conferences
AstronomyPhysics
2015English

DNA Fragmentation in Microorganisms Assessed in Situ

Applied and Environmental Microbiology
Applied MicrobiologyBiotechnologyEcologyFood Science
2008English

The Abundance of Boron in Disk-Metallicity Stars

Symposium - International Astronomical Union
2000English

Fe-Peak Element Abundances in Disk and Halo Stars

Proceedings of the International Astronomical Union
AstrophysicsAstronomyPlanetary ScienceSpace
2009English

Amanote Research

Note-taking for researchers

Follow Amanote

© 2025 Amaplex Software S.P.R.L. All rights reserved.

Privacy PolicyRefund Policy