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Near infrared adaptive optics observations are crucial to be able to interpret kinematic and dynamical data and study star formation properties within the often extremely dusty interacting luminous IR galaxies (LIRGs). NIR AO data are also…

Cosmology and Nongalactic Astrophysics · Physics 2009-08-26 Petri Vaisanen , Seppo Mattila , Stuart Ryder

We present a study of the stellar populations of ring and/or arm-like structures in a sample of S0 galaxies using GALEX far- and near-ultraviolet imaging and SDSS optical data. Such structures are prominent in the UV and reveal recent star…

Cosmology and Nongalactic Astrophysics · Physics 2015-03-17 A. Marino , L. Bianchi , R. Rampazzo , D. Thilker , F. Annibali , A. Bressan , L. M. Buson

Polar-ring galaxies are systems with two nearly orthogonal rotational axes, and are therefore clearly the result of galaxy-galaxy interactions. The host galaxies of polar rings are typically gas-poor early-type systems. The rings…

Astrophysics · Physics 2007-05-23 Paul B. Eskridge , Richard W. Pogge

Star formation in galaxies is observed to be associated with gamma-ray emission. The detection of gamma rays from star-forming galaxies by the Fermi Large Area Telescope (LAT) has allowed the determination of a functional relationship…

High Energy Astrophysical Phenomena · Physics 2012-08-07 Emma Storm , Tesla E. Jeltema , Stefano Profumo

With the help of a statistical parameter derived from optical spectra, we show that the current star formation rate of a galaxy, falling into a cluster along a supercluster filament, is likely to undergo a sudden enhancement before the…

We have mapped the inner 360'' regions of M51 in the 158micron [CII] line at 55'' spatial resolution using the Far-infrared Imaging Fabry-Perot Interferometer (FIFI) on the Kuiper Airborne Observatory (KAO). The emission is peaked at the…

Astrophysics · Physics 2009-11-06 T. Nikola , N. Geis , F. Herrmann , S. C. Madden , A. Poglitsch , G. J. Stacey , C. H. Townes

Images of 7 Compact groups of galaxies (CG) were obtained using the 2.1m telescope in San Pedro Martir (B.C. Mexico) equipped with the NIR camera CAMILA. The NIR images trace the mass of the galaxies, through the oldest and more evolved…

Astrophysics · Physics 2015-06-24 I. Plauchu-Frayn , R. Coziol , H. Bravo-Alfaro

We present GALEX NUV (2310 A) and FUV (1530 A) images of the interacting galaxy NGC 4438 (Arp 120) in the center of the Virgo cluster. These images show an extended (20 kpc) tidal tail at the north-west edge of the galaxy previously…

We study star formation in a sample of 1204 galaxies in minor (| \Delta m_z | \geq 2) pairs and compact groups, drawn from the Sloan Digital Sky Survey Data Release 5 (SDSS DR5). We analyze an analogous sample of 2409 galaxies in major (|…

Astrophysics · Physics 2008-11-26 Deborah Freedman Woods , Margaret J. Geller

We present high-resolution radio continuum observations of the nascent starburst in the metal-poor galaxy SBS 0335-052. These radio data were taken with the Very Large Array and include observations at 0.7cm, 1.3cm, 2cm, 3.6cm, and 6cm.…

Cosmology and Nongalactic Astrophysics · Physics 2009-11-13 K. E. Johnson , L. K. Hunt , A. E. Reines

New spectral line observations, obtained with the Jansky Very Large Array (VLA), of a sample of 34 galaxies in 17 close pairs are presented in this paper. The sample of galaxy pairs is selected to contain galaxies in close, major…

We analyzed HST images of 31 nearby (z <~ 0.1) 3CR radio-galaxies. We compared their UV and optical images to detect evidence of recent star formation. Six objects were excluded because they are highly nucleated or had very low UV count…

Astrophysics · Physics 2009-11-13 Ranieri D. Baldi , Alessandro Capetti

We assemble a sample of 733 dwarf galaxies ($M_{\ast} \le 10^{9.5} \text{M}_\odot$) with signatures of active galactic nuclei (AGN) and explore the intersection between different AGN selection techniques. Objects in our database are…

Astrophysics of Galaxies · Physics 2024-05-31 Erik J. Wasleske , Vivienne F. Baldassare

Merger processes play an important role in galaxy formation and evolution. To study the influence of merger processes on the evolution of dust properties and cosmic star formation rate, we investigate a local sample of major merger galaxies…

Cosmology and Nongalactic Astrophysics · Physics 2012-12-11 F. -T. Yuan , T. T. Takeuchi , Y. Matsuoka , V. Buat , D. Burgarella , J. Iglesias-Páramo

We introduce a near-IR monitoring campaign of the Local Group spiral galaxy M33, carried out with the UK IR Telescope (UKIRT). The pulsating giant stars are identified and their distributions are used to derive the star formation rate as a…

Astrophysics of Galaxies · Physics 2011-01-28 Atefeh Javadi , Jacco Th. van Loon , Mohammad Taghi Mirtorabi

We have performed a comprehensive study of the UV emission detected from AGB stars by the Galaxy Evolution Explorer (GALEX). Of the 468 AGB stars in our sample, 316 were observed by GALEX. In the NUV bandpass ($\lambda_{\rm eff} \sim 2310$z…

Solar and Stellar Astrophysics · Physics 2017-05-31 Rodolfo Montez , Sofia Ramstedt , Joel H. Kastner , Wouter Vlemmings , Enmanuel Sanchez

We study the UV properties of a volume limited sample of early-type galaxies in the Virgo cluster combining new GALEX far- (1530 A) and near-ultraviolet (2310 A) data with spectro-photometric data available at other wavelengths. The sample…

Solar-type members of the rich, nearly Solar-age and Solar-metallicity M67 open cluster are systematically investigated for ultraviolet variability. We utilize archival Galaxy Evolution Explorer (GALEX) data which features several imaging…

Solar and Stellar Astrophysics · Physics 2025-05-20 Carl Melis , Ekamjot Kaire

We present a novel approach for classifying star-forming galaxies using photometric images. By utilizing approximately $124,000$ optical color composite images and spectroscopic data of nearby galaxies at $0.01<z<0.06$ from the Sloan…

Astrophysics of Galaxies · Physics 2025-08-01 Kyuseok Oh , M. Dennis Turp

We present deep observations taken with the HST Advanced Camera for Surveys of the central massive galaxy in a forming cluster at z=2.2. The galaxy hosting the powerful radio source MRC 1138-262 is associated with one of the most extensive…

Astrophysics · Physics 2008-11-26 Roderik A. Overzier , George K. Miley , Holland C. Ford