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Related papers: Ongoing Massive Star Formation in NGC 604

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We present observations of 1.2-mm dust continuum emission, made with the Swedish ESO Submillimeter Telescope, towards eighteen luminous IRAS point sources, all with colors typical of compact HII regions and associated with CS(2-1) emission,…

Astrophysics · Physics 2011-02-11 Guido Garay , Diego Mardones , Kate J. Brooks , Liza Videla , Yanett Contreras

The total-to-selective extinction RV in the direction of a cluster is found to be 3.12 +/- 0.2 (close to its normal value). We derive the luminosity and mass functions for the cluster main sequence stars. The mass function slope is found to…

Solar and Stellar Astrophysics · Physics 2015-12-14 Gireesh C. Joshi

Massive stars form on different scales ranging from large, dispersed OB associations to compact, dense starburst clusters. The complex structure of regions of massive star formation, and the involved short timescales provide a challenge for…

Astrophysics of Galaxies · Physics 2016-04-06 Shi-Wei Wu , Arjan Bik , Joachim M. Bestenlehner , Thomas Henning , Anna Pasquali , Wolfgang Brandner , Andrea Stolte

NGC 6791 is an old, metal-rich star cluster normally considered to be a disk open cluster. Its red giant branch is broad in color yet, to date, there is no evidence for a metallicity spread among its stars. The turnoff region of the main…

Solar and Stellar Astrophysics · Physics 2015-05-20 Bruce A. Twarog , Giovanni Carraro , Barbara J. Anthony-Twarog

We present high spatial resolution (0.6 arcsec) near-infrared broad-band JHK images and Br_gamma 2.1661 micron and H_2 1-0 S(1) 2.122 micron emission line images of the nuclear regions in the interacting starburst galaxies NGC 520, NGC 1614…

Astrophysics · Physics 2009-10-31 J. K. Kotilainen , J. Reunanen , S. Laine , S. D. Ryder

With an extinction-corrected V-band peak absolute magnitude of about -22, supernova (SN) 2006gy is probably the brightest SN ever observed. We report on multi-wavelength observations of this SN and its environment. Our spectroscopy shows an…

We present radio and infrared observations indicating on-going star formation activity inside the $\sim2-5$ pc circumnuclear ring at the Galactic center. Collectively these measurements suggest a continued disk-based mode of on-going star…

Astrophysics of Galaxies · Physics 2015-08-06 F. Yusef-Zadeh , M. Wardle , M. Sewilo , D. A. Roberts , I. Smith , R. Arendt , W. Cotton , J. Lacy , S. Martin , M. W. Pound , M. Rickett , M. Royster

We present a multi-wavelength study to analyse the star formation process associated with the mid-infrared bubble CN 148 (H II region G10.3-0.1), which harbors an O5V-O6V star. The arc-shaped distribution of molecular CO(2-1) emission, the…

Astrophysics of Galaxies · Physics 2015-06-23 L. K. Dewangan , D. K. Ojha , J. M. C. Grave , K. K. Mallick

The Massive Young star-forming complex Study in Infrared and X-ray (MYStIX) uses data from the Chandra X-ray Observatory to identify and characterize the young stellar populations in twenty Galactic (d < 4 kpc) massive star-forming regions.…

Solar and Stellar Astrophysics · Physics 2016-11-25 Michael A. Kuhn , Konstantin V. Getman , Patrick S. Broos , Leisa K. Townsley , Eric D. Feigelson

We present new Hubble Space Telescope (HST) observations of NGC 300 taken as part of the ACS Nearby Galaxy Survey Treasury (ANGST). Individual stars are resolved in these images down to an absolute magnitude of M_F814W = 1.0 (below the red…

Massive galaxies in the early Universe have been shown to be forming stars at surprisingly high rates. Prominent examples are dust-obscured galaxies which are luminous when observed at sub-millimeter (sub-mm) wavelengths and which may be…

High resolution, 1.1, 1.6, and 2.2 micron imaging of the luminous infrared galaxy NGC 6090 obtained with NICMOS of the Hubble Space Telescope are presented. These new observations are centered on the two nuclei of the merger, and reveal the…

Astrophysics · Physics 2009-10-31 N. Dinshaw , A. S. Evans , H. Epps , N. Z. Scoville , M. Rieke

We present multi-wavelength analysis around mid-infrared bubble N14 to probe the signature of triggered star formation as well as the formation of new massive star(s) and/or cluster(s) on the borders of the bubble by the expansion of the H…

Astrophysics of Galaxies · Physics 2015-06-12 L. K. Dewangan , D. K. Ojha

We present new H alpha and [O III] 5007 narrow band images of the starbursting dwarf galaxy NGC 4214, obtained with the WFPC2 onboard HST, together with VLA observations of the same galaxy. The HST images resolve features down to physical…

We present images and initial results from our extensive Spitzer Space Telescope imaging survey of the W5 H II region with the Infrared Array Camera (IRAC) and Multiband Imaging Photometer for Spitzer (MIPS). We detect dense clusters of…

We present new mid-infrared N-band spectroscopy and Q-band photometry of the local luminous infrared galaxy NGC1614, one of the most extreme nearby starbursts. We analyze the mid-IR properties of the nucleus (central 150 pc) and four…

We present multicolor photometry of bright star cluster candidates in the nearby starburst galaxies NGC 3077 and NGC 5253, observed with the Hubble Space Telescope Wide Field and Planetary Camera 2 in both broadband (F300W, F547M and F814W)…

Astrophysics · Physics 2009-11-10 J. Harris , D. Calzetti , J. S. Gallagher , D. A. Smith , C. J. Conselice

The bright Type II-plateau supernova (SN) 2004dj occurred within the young, massive stellar cluster Sandage-96 in a spiral arm of NGC 2403. New multi-wavelength observations obtained with several ground-based and space-based telescopes are…

Rings in S0s are enigmatic features which can however betray the evolutionary paths of particular galaxies. We have undertaken long-slit spectroscopy of five lenticular galaxies with UV-bright outer rings. The observations have been made…

Astrophysics of Galaxies · Physics 2019-06-19 Irina S. Proshina , Alexei Yu. Kniazev , Olga K. Sil'chenko

We examine the thirteen most luminous sources in the WMAP free-free map using the Spitzer GLIMPSE and MSX surveys to identify massive star formation regions, emitting one-third of the Galactic free-free luminosity. We identify star forming…

Astrophysics of Galaxies · Physics 2010-07-28 Mubdi Rahman , Norman Murray