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相关论文: A deep dive into NGC 604 with Gemini/NIRI imaging

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The current state-of-the-art of multi-wavelength diagnostic tools (evolutionary synthesis, photoionisation models) for massive star forming regions (HII regions, starbursts, etc.) and some of their input physics (especially model…

天体物理学 · 物理学 2007-05-23 Daniel Schaerer

We present very deep CCD spectrum of the bright, medium-excitation planetary nebula NGC 7009, with a wavelength coverage from 3040 to 11000 A. Traditional emission line identification is carried out to identify all the emission features in…

太阳与恒星天体物理 · 物理学 2015-05-27 X. Fang , X. -W. Liu

The upper region of the Hertzsprung-Russell diagram is populated by massive stars in a diversity of evolutionary stages, and the classification of these stars is often based on observed characteristics exclusively in the optical spectral…

太阳与恒星天体物理 · 物理学 2025-07-28 Michaela Kraus , Maria Laura Arias , Michalis Kourniotis , Andrea Torres , Lydia S. Cidale , Marcelo Borges Fernandes

We have used the Gemini Near-infrared Integral Field Spectrograph (NIFS) to map the emission-line intensity distributions and ratios in the Narrow-Line Region (NLR) of the Seyfert galaxy NGC 4151 in the Z, J, H and K bands at a resolving…

天体物理学 · 物理学 2009-11-13 T. Storchi-Bergmann , P. J. McGregor , Rogemar A. Riffel , R. Simoes-Lopes , T. Beck , M. Dopita

We present Gemini-S/GMOS-IFU optical spectroscopy of four regions near the centre of the nearby (3.8 Mpc) dwarf starburst galaxy NGC 5253. This galaxy is famous for hosting a radio supernebula containing two deeply embedded massive super…

宇宙学与河外天体物理 · 物理学 2015-06-12 M. S. Westmoquette , B. James , A. Monreal-Ibero , J. R. Walsh

Deep, near-infrared imaging surveys have been motivated by the desire to study the rest-frame optical properties and stellar content of galaxies at high redshift. Here we briefly review their history, and illustrate one application, using…

天体物理学 · 物理学 2009-11-06 Mark Dickinson , Casey Papovich , Henry C. Ferguson

We present a multiwavelength investigation of the HII region G25.8700+0.1350, located in the inner part of the Galaxy. In radio continuum emission, the region is seen as a bright arc-shaped structure. An analysis of the HI line suggests…

星系天体物理 · 物理学 2017-12-20 S. Cichowolski , N. U. Duronea , L. A. Suad , E. M. Reynoso , R. Dorda

We report the discovery of a confirmed supernova (SN) and a supernova-candidate in near-infrared images from the ALTAIR/NIRI adaptive optics system on the Gemini-North Telescope and NICMOS on the Hubble Space Telescope. The Gemini images…

We present a near-infrared study of the Seyfert 2 galaxy NGC\,6300, based on subarcsecond images and long slit spectroscopy obtained with Flamingos-2 at Gemini South. We have found that the peak of the nuclear continuum emission in the…

星系天体物理 · 物理学 2019-02-08 Gaia Gaspar , Rubén Díaz , Damián Mast , Ary D'Ambra , María Paz Agüero , Guillermo Günthardt

The neighborhood of the Galactic black hole boasts a plethora of extended interstellar gas and dust features as well as populations of compact (unresolved, or marginally resolved) features such as the G objects. Most are well manifested in…

星系天体物理 · 物理学 2023-11-29 Cuc K. Dinh , Anna Cuirlo , Mark R. Morris , Rainer Schödel , Andrea Ghez , Tuan Do

We present H-band images obtained with NICMOS of a field 75'' (5kpc) above the plane of the disk of the edge-on spiral galaxy NGC 5907. Ground-based observations have shown that NGC 5907 has a luminous halo with a shallow radial profile…

天体物理学 · 物理学 2009-10-31 Stephen E. Zepf , Michael C. Liu , Francine R. Marleau , Penny D. Sackett , James. R. Graham

Far-infrared line and continuum fluxes are presented for a sample of 227 galaxies observed with the Long Wavelength Spectrometer on the Infrared Space Observatory. The galaxy sample includes normal star-forming systems, starbursts, and…

天体物理学 · 物理学 2009-11-13 James R. Brauher , Daniel A. Dale , George Helou

During pilot observations of the Virgo Environmental Survey Tracing Galaxy Evolution (VESTIGE), a blind narrow-band Halpha+[NII] imaging survey of the Virgo cluster carried out with MegaCam at the CFHT, we have observed the spiral galaxy…

We present the first results from a 124 night J, H, K near-infrared monitoring campaign of the dark cloud L 1003 in Cygnus OB7, an active star-forming region. Using 3 seasons of UKIRT observations spanning 1.5 years, we obtained…

太阳与恒星天体物理 · 物理学 2015-06-05 Thomas S. Rice , Scott J. Wolk , Colin Aspin

NGC 4449 is an irregular galaxy with a moderately high star formation activity. The massive stars in NGC 4449 have given rise to many bright HII regions, superbubbles, supergiant shells, and "chimney-like" radial filaments. ROSAT X-ray…

天体物理学 · 物理学 2009-10-30 D. J. Bomans , Y. -H. Chu , U. Hopp

In this paper we present the results of a mid infrared study of G49.5-0.4, or W51A, part of the massive starbirth complex W51. Combining public data from the $Spitzer$ IRAC camera, and Gemini mid infrared camera T-ReCS at 7.73, 9.69, 12.33…

星系天体物理 · 物理学 2016-07-06 Cassio L. Barbosa , Robert D. Blum , Augusto Damineli , Peter S. Conti , Danilo M. Gusmão

We present the results of the Gemini Deep Planet Survey, a near-infrared adaptive optics search for giant planets and brown dwarfs around nearby young stars. The observations were obtained with the Altair adaptive optics system at the…

Combining the relative vicinity of the Local Group spiral galaxy M33 with the Spitzer images, we investigate the properties of infrared (IR) emission sites and assess the reliability of the IR emission as a star formation tracer. The mid-…

天体物理学 · 物理学 2009-11-13 S. Verley , L. K. Hunt , E. Corbelli , C. Giovanardi

The nearby irregular galaxy NGC4449 has a star formation rate of about 0.4 solar masses/yr and should host of order 70 SNRs younger than 20,000 years, a typical age for SNRs expanding into to an ISM with unit density to reach the radiative…

星系天体物理 · 物理学 2023-10-09 P. Frank Winkler , Knox S. Long , William P. Blair