Results 111 to 120 of about 849,819 (226)

The Multiple Extended Tidal Tails of NGC 288

open access: yesThe Astrophysical Journal
Using photometry and proper motions from Pan-STARRS, DECaLS, and Gaia Data Release 3, we detect a ∼35°–70° long trailing stellar debris stream associated with the globular cluster NGC 288.
Carl J. Grillmair
doaj   +1 more source

A Neutral Hydrogen Absorption Study of Cold Gas in the Outskirts of the Magellanic Clouds Using the GASKAP-H i Survey

open access: yesThe Astronomical Journal
Cold neutral hydrogen (H i ) is a crucial precursor for molecular gas formation and can be studied via H i absorption. This study investigates H i absorption in low column density regions of the Small and Large Magellanic Clouds (SMC and LMC) using the ...
Hongxing Chen   +20 more
doaj   +1 more source

The Magellanic Stream in Modified Newtonian Dynamics

open access: yes, 2006
The dynamics of the Magellanic Stream (MS) as a series of clouds extending from the Magellanic Clouds (MCs) to the south Galactic pole is affected by the distribution and the amount of matter in the Milky Way. We calculate the gravitational effect of the
Haghi, Hossein   +2 more
core   +1 more source

Streams, Shells, and Substructures in the Accretion-built Stellar Halo of NGC 300

open access: yesThe Astrophysical Journal Letters
We present deep optical observations of the stellar halo of NGC 300, an LMC-mass galaxy, acquired with the DEEP subcomponent of the DECam Local Volume Exploration survey using the 4 m Blanco Telescope.
Catherine E. Fielder   +29 more
doaj   +1 more source

Metal Abundances in the Magellanic Stream

open access: yesThe Astronomical Journal, 2000
We report on the first metallicity determination for gas in the Magellanic Stream, using archival HST GHRS data for the background targets Fairall 9, III Zw 2, and NGC 7469. For Fairall 9, using two subsequent HST revisits and new Parkes Multibeam Narrowband observations, we have unequivocally detected the MSI HI component of the Stream (near its head)
Gibson, Brad K.   +5 more
openaire   +2 more sources

Spatial motion of the Magellanic Clouds. Tidal models ruled out?

open access: yes, 2008
Recently, Kallivayalil et al. derived new values of the proper motion for the Large and Small Magellanic Clouds (LMC and SMC, respectively). The spatial velocities of both Clouds are unexpectedly higher than their previous values resulting from agreement
Palous, Jan   +2 more
core   +1 more source

The Role of Dwarf Galaxy Interactions in Shaping the Magellanic System and Implications for Magellanic Irregulars

open access: yes, 2012
We present a novel pair of numerical models of the interaction history between the Large and Small Magellanic Clouds (LMC and SMC, respectively) and our Milky Way (MW) in light of recent high precision proper motions (Kallivayalil et al. 2006a,b).
Agertz   +161 more
core   +1 more source

The disruption of the Magellanic Stream [PDF]

open access: yesProceedings of the International Astronomical Union, 2008
AbstractWe present evidence that the accretion of warm gas onto the Galaxy today is at least as important as cold gas accretion. For more than a decade, the source of the bright Hα emission (up to 750 mR†) along the Magellanic Stream has remained a mystery.
openaire   +1 more source

Charting the Galactic Acceleration Field. II. A Global Mass Model of the Milky Way from the STREAMFINDER Atlas of Stellar Streams Detected in Gaia DR3

open access: yesThe Astrophysical Journal
We present an atlas and follow-up spectroscopic observations of 87 thin stream-like structures detected with the STREAMFINDER algorithm in Gaia DR3, of which 28 are new discoveries.
Rodrigo Ibata   +19 more
doaj   +1 more source

The Escape of Ionizing Photons from the Galaxy

open access: yes, 1998
The Magellanic Stream and several high velocity clouds have now been detected in optical line emission. The observed emission measures and kinematics are most plausibly explained by photoionization due to hot, young stars in the Galactic disk. The highly
Giallongo E.   +4 more
core   +1 more source

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