Results 61 to 70 of about 339,165 (211)

The Herschel Dwarf Galaxy Survey - I. Properties of the low-metallicity ISM from PACS spectroscopy [PDF]

open access: yes, 2015
Context. The far-infrared (FIR) lines are important tracers of the cooling and physical conditions of the interstellar medium (ISM) and are rapidly becoming workhorse diagnostics for galaxies throughout the universe.
D. Cormier   +20 more
semanticscholar   +1 more source

Dust in Nearby DWARF Galaxies [PDF]

open access: yesSymposium - International Astronomical Union, 1994
The aim of the present paper is to look for the gas-to-dust ratio in different types of galaxies and for a correlation between this ratio and the metallicity in dwarf galaxies. The recent compilation of data on nearby galaxies by Schmidt & Boller (1992, hereinafter SB) including HI and dust ...
K.-H. Schmidt, T. Boller
openaire   +1 more source

An Accreting Supermassive Black Hole Buried in a Faint Dwarf Galaxy

open access: yesThe Astrophysical Journal Letters
In the last decade, there have been several discoveries of active galactic nuclei (AGN) in dwarf galaxies including an AGN in an ultracompact dwarf galaxy with a black hole mass >10 ^6 M _⊙ .
Abhishek Paswan, Mousumi Das, K Rubinur
doaj   +1 more source

The unexpected diversity of dwarf galaxy rotation curves [PDF]

open access: yes, 2015
We examine the circular velocity profiles of galaxies in A cold dark matter (CDM) cosmological hydrodynamical simulations from the EAGLE and LOCAL GROUPS projects and compare them with a compilation of observed rotation curves of galaxies spanning a wide
K. Oman   +11 more
semanticscholar   +1 more source

Star Forming Dwarf Galaxies [PDF]

open access: yes, 2011
Star forming dwarf galaxies (SFDGs) have a high gas content and low metallicities, reminiscent of the basic entities in hierarchical galaxy formation scenarios. In the young universe they probably also played a major role in the cosmic reionization. Their abundant presence in the local volume and their youthful character make them ideal objects for ...
openaire   +2 more sources

STELLAR KINEMATICS AND METALLICITIES IN THE ULTRA-FAINT DWARF GALAXY RETICULUM II [PDF]

open access: yes, 2015
We present Magellan/M2FS, Very Large Telescope/GIRAFFE, and Gemini South/GMOS spectroscopy of the newly discovered Milky Way satellite Reticulum II. Based on the spectra of 25 Ret II member stars selected from Dark Energy Survey imaging, we measure a ...
J. Simon   +79 more
semanticscholar   +1 more source

Discovery of a Double-core Dwarf Galaxy in a Major Wet Merger: MCG+08-16-005

open access: yesThe Astronomical Journal
I present the discovery of a dwarf galaxy with double cores, MCG+08-16-005, observed by an Integral Field Unit. Based on photometric and spatially resolved spectroscopic analyses, the galaxy is suggested as an ongoing dwarf-dwarf merger. MCG+08-16-005 is
Youngdae Lee
doaj   +1 more source

DGSAT: Dwarf Galaxy Survey with Amateur Telescopes I. Discovery of low surface brightness systems around nearby spiral galaxies [PDF]

open access: yes, 2015
Context: We introduce the Dwarf Galaxy Survey with Amateur Telescopes (DGSAT) project and report the discovery of eleven low surface brightness (LSB) galaxies in the fields of the nearby galaxies NGC 2683, NGC 3628, NGC 4594 (M104), NGC 4631, NGC 5457 ...
B. Javanmardi   +11 more
semanticscholar   +1 more source

New dwarf galaxy candidates in the Centaurus group [PDF]

open access: yes, 2015
Recent studies of the distribution and kinematics of the Milky Way and Andromeda satellite galaxy systems have confirmed the existence of coplanar, corotating structures of galaxies. In addition to the 'missing satellite problem', these structures pose a
O. Muller, H. Jerjen, B. Binggeli
semanticscholar   +1 more source

Energy Evolution in the Progenitor of Galaxy Shells: A Semi-analytical Model

open access: yesThe Astrophysical Journal
The stellar shells surrounding an elliptical galaxy, as remnants of a dwarf galaxy disrupted during merging, reveal the distribution of energy and angular momentum of the progenitor dwarf galaxy. We develop a semi-analytical model to describe the changes
Beibei Guo   +3 more
doaj   +1 more source

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