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We present low resolution (R~450) K-band spectroscopy for 16 of the 43 circumnuclear star-forming knots in M100 identified by Ryder & Knapen (1999). We compare our measurements of equivalent widths for the Br-gamma emission line and CO 2.29…

Astrophysics · Physics 2015-06-24 S. D. Ryder , J. H. Knapen , M. Takamiya

High-resolution NIR and optical images are used to constrain a dynamical model of the circumnuclear star forming (SF) region in the barred galaxy M100 (=NGC 4321). Subarcsecond resolution allowed us to distinguish important morphological…

Astrophysics · Physics 2019-07-31 J. H. Knapen , R. F. Peletier , I. Shlosman , J. E. Beckman , C. H. Heller , R. S. de Jong

We present new high-resolution observations of the center of the late-type spiral M100 (NGC 4321) supplemented by 3D numerical modeling of stellar and gas dynamics, including star formation (SF). NIR imaging has revealed a stellar bar,…

Astrophysics · Physics 2010-04-21 J. H. Knapen , J. E. Beckman , C. H. Heller , I. Shlosman , R. S. de Jong

I discuss new observations of circumnuclear regions in barred galaxies, both of their kinematics and their near-infrared (NIR) morphology. New kinematic observations of M100 confirm that (1) the inner bar-like feature detected before in…

Astrophysics · Physics 2015-06-24 Johan H. Knapen

We present sub-arcsecond resolution ground-based near-infrared images of the central regions of a sample of twelve barred galaxies with circumnuclear star formation activity, which is organized in ring-like regions typically one kiloparsec…

Astrophysics · Physics 2009-10-31 D. Perez-Ramirez , J. H. Knapen , R. F. Peletier , S. Laine , R. Doyon , D. Nadeau

We present infrared and radio continuum observations of S 201 star forming region. A massive star cluster is observed in this region, which contains different classes of young stellar objects. The near-infrared colour-colour and…

Astrophysics · Physics 2009-11-10 D. K. Ojha , S. K. Ghosh , V. K. Kulkarni , L. Testi , R. P. Verma , S. Vig

We present ISOCAM images (1.5"/px) in the LW2 (6.75 microns) and LW3 (15 microns) broad band filters of the circumnuclear starburst of NGC 4321 (M 100). A detailed comparison with the emission at other wavelengths (U, B, Halpha, and CO) is…

Astrophysics · Physics 2007-05-23 H. Wozniak , D. Friedli , L. Martinet , D. Pfenniger

We present photometry in U, B, V, R and I continuum bands and in H$\alpha$ and H$\beta$ emission lines for a sample of 336 circumnuclear star forming regions (CNSFR) located in early type spiral galaxies with different levels of activity in…

Astrophysics of Galaxies · Physics 2017-01-04 Mar Álvarez-Álvarez , Angeles I. Díaz , Elena Terlevich , Roberto Terlevich

(Abridged) Star-forming nuclear rings in barred galaxies are common in nearby spirals, and their detailed study can lead to important insights into the evolution of galaxies, their bars, and their central regions. We present integral field…

Astrophysics · Physics 2009-11-11 Emma L. Allard , Johan H. Knapen , Reynier F. Peletier , Marc Sarzi

New optical and NIR K-band images of the inner 3 kpc region of the nearby Virgo spiral M100 (NGC 4321) display remarkable morphological changes with wavelength. While in the optical the light is dominated by a circumnuclear zone of enhanced…

Astrophysics · Physics 2009-10-28 J. H. Knapen , J. E. Beckman , I. Shlosman , R. F. Peletier , C. H. Heller , R. S. de Jong

Star formation is a clustered process that regulates the structure and evolution of galaxies. We investigate this process in the dwarf galaxy Haro 11, forming stars in three knots (A, B, C). The exquisite resolution of HST imaging allows us…

Astrophysics of Galaxies · Physics 2022-01-19 M. Sirressi , A. Adamo , M. Hayes , A. Bik , M. Strandänger , A. Runnholm , M. S. Oey , G. Östlin , V. Menacho , L. J. Smith

We have conducted a near-infrared monitoring campaign at the UK InfraRed Telescope (UKIRT), of the Local Group spiral galaxy M33 (Triangulum). The main aim was to identify stars in the very final stage of their evolution, and for which the…

Solar and Stellar Astrophysics · Physics 2015-05-27 Atefeh Javadi , Jacco Th. van Loon , Mohammad Taghi Mirtorabi

Images of IRAS galaxies with a range of IR properties are examined for bright knots, both within and outside the galaxy. These are found almost exclusively in galaxies with steep IR spectra, but over a wide range of IR luminosity, and…

Astrophysics · Physics 2009-10-28 J. B. Hutchings

The SAURON integral field spectrograph was used to observe the central area of the barred spiral galaxy M100 (NGC 4321). M100 contains a nuclear ring of star formation, fueled by gas channeled inward by the galaxy's bar. We present maps of…

Astrophysics · Physics 2009-11-13 Emma L. Allard , Reynier F. Peletier , Johan H. Knapen

All slightly extended sources were identified on deep K-band maps of 46 spiral galaxies reaching at least K=20.3 mag/arcsec2 at a signal-to-noise level of 3. The galaxies had inclination angles <65 deg and linear resolutions <100 pc with…

Astrophysics · Physics 2008-09-24 P. Grosbol , H. Dottori

NGC 5291, an early-type galaxy surrounded by a giant HI ring, is believed to be formed from collision with another galaxy. Several star forming complexes and tidal dwarf galaxies are distributed along the collisional ring which are sites of…

Using HST WFPC2 images, we have obtained U, B, V, I, and H-alpha photometry for 76 star clusters in the nuclear star-forming ring of the barred spiral galaxy NGC 4314. These clusters are likely associated with an inner Inner Lindblad…

We present high spatial resolution H and K'-band images of a complete sample of ultraluminous infrared galaxies selected to have warm mid-infrared colors known to be characteristic of active galaxies. The extended underlying galaxy is…

Astrophysics · Physics 2009-10-30 Jason A. Surace , D. B. Sanders

We present UV (2300 Ang) images, obtained with the HST Faint Object Camera, of the central 20'' of five galaxies containing circumnuclear star-forming rings. The five galaxies are from a well-defined sample of 103 normal, nearby galaxies we…

The composite galaxy NGC 4102 hosts a LINER nucleus and a starburst. We mapped NGC 4102 in the 12.8 micron line of [NeII], using the echelon spectrometer TEXES on the NASA IRTF, to obtain a data cube with 1.5" spatial and 25 km/s spectral,…

Astrophysics of Galaxies · Physics 2015-05-19 Sara C. Beck , John H. Lacy , Jean L. Turner
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