Results 61 to 70 of about 10,431 (186)
Intermediate Mass Ratio Inspirals in Milky Way Galaxies
A consequence of a nonzero occupation fraction of massive black holes (MBHs) in dwarf galaxies is that these MBHs can become residents of larger galaxy halos via hierarchical merging and tidal stripping.
Jillian Bellovary +5 more
doaj +1 more source
Angular momentum content in gas-rich dwarf galaxies [PDF]
Aditya Chowdhury, Jayaram N. Chengalur
openalex +1 more source
We are entering an era in which we will be able to detect and characterize hundreds of dwarf galaxies within the Local Volume. It is already known that a strong dichotomy exists in the gas content and star formation properties of field dwarf galaxies ...
Charlotte R. Christensen +7 more
doaj +1 more source
KMTNet Nearby Galaxy Survey II. Searching for Dwarf Galaxies in Deep and Wide-field Images of the NGC 1291 System [PDF]
Woowon Byun +13 more
openalex +1 more source
We investigate the connection between accretion signatures and host galaxy properties in the context of how active dwarf galaxies are identified. We use the database constructed in E. J. Wasleske & V. F.
Erik J. Wasleske +2 more
doaj +1 more source
FUSE observations of the Blue Compact Dwarf Galaxy Mrk 59 [PDF]
T. X. Thuan +2 more
openalex +1 more source
Chemical Cartography of the Sagittarius Stream with Gaia
The stellar stream connected to the Sagittarius (Sgr) dwarf galaxy is the most massive tidal stream that has been mapped in the Galaxy, and is the dominant contributor to the outer stellar halo of the Milky Way (MW).
Emily C. Cunningham +7 more
doaj +1 more source
87th Annual Meeting of the Meteoritical Society 2025: Abstracts
Meteoritics &Planetary Science, Volume 60, Issue S1, Page 30-350, August 2025.
wiley +1 more source
Recent efforts have extended our view of the number and properties of satellite galaxies beyond the Local Group firmly down to M _⋆ ∼ 10 ^6 M _⊙ . A similarly complete view of the field dwarf population has lagged behind.
Erin Kado-Fong +10 more
doaj +1 more source
A spectroscopic study of the merging dwarf galaxy PGC 007782
We did a detailed spectroscopic study of PGC 007782, an interacting emission type dwarf galaxy. This study utilized the optical spectrum of emission lines to explore the system of interacting dwarf galaxies.
Shankar Timalsina, Daya Nidhi Chhatkuli
doaj +1 more source

