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NGC 2359 is a Wolf-Rayet (W-R) nebula partially bound by a rather dense and warm molecular cloud. We present the results derived from CO and $^{13}$CO fully sampled maps of the molecular material with angular resolutions up to 12". We have…

Astrophysics · Physics 2009-11-10 J. R. Rizzo , J. Martin-Pintado , J. -F. Desmurs

The halos of disk galaxies form a crucial connection between the galaxy disk and the intergalactic medium. Massive stars, HII regions, or dwarf galaxies located in the halos of galaxies are potential tracers of recent accretion and/or…

Astrophysics of Galaxies · Physics 2018-11-28 Y. Stein , D. J. Bomans , P. Kamphuis , E. Jütte , M. Langener , R. -J. Dettmar

We present results of long-slit and panoramic spectroscopy of extended gaseous disks in 18 nearby S0 galaxies, mostly in groups. The gas in our S0s is found to be often accreted from outside that is implied by its decoupled kinematics: at…

Astrophysics of Galaxies · Physics 2019-09-11 Olga K. Sil'chenko , Alexei V. Moiseev , Oleg V. Egorov

We present optical and near-IR imaging and spectroscopy of SGAS J105039.6$+$001730, a strongly lensed galaxy at z $=$ 3.6252 magnified by $>$30$\times$, and derive its physical properties. We measure a stellar mass of…

Cosmology and Nongalactic Astrophysics · Physics 2015-06-17 Matthew B. Bayliss , Jane R. Rigby , Keren Sharon , Eva Wuyts , Michael Florian , Michael D. Gladders , Traci Johnson , Masamune Oguri

Using the combined resolving power of the Hubble Space Telescope and gravitational lensing, we resolve star-forming structures in a z~2.5 galaxy on scales much smaller than the usual kiloparsec diffraction limit of HST. SGAS…

(Abridged) We perform a comprehensive multiwavelength analysis of a sample of 20 starburst galaxies that show the presence of a substantial population of Wolf-Rayet (WR) stars. In this paper we present the analysis of the O and WR star…

Cosmology and Nongalactic Astrophysics · Physics 2015-05-18 Angel R. Lopez-Sanchez , Cesar Esteban

Our new survey for Wolf-Rayet stars in the Magellanic Clouds is only 15% complete but has already found 9 new WRs in the LMC. This suggests that the total WR population in the LMC may be underestimated by 10-40%. Eight of the nine are WNs,…

Solar and Stellar Astrophysics · Physics 2015-06-22 Philip Massey , Kathryn F. Neugent , Nidia Morrell , D. John Hillier

The star formation histories of Local Group (LG) dwarf galaxies and more distant potential LG members are reviewed. Problems in defining the spatial extent of the LG and membership are briefly discussed. The morphological types found in the…

Astrophysics · Physics 2007-05-23 Eva K. Grebel

Wolf-Rayet stars (WRs) are very important massive stars. However, their origin and the observed binary fraction within the entire WR population are still debated. We investigate some possible merger channels for the formation of WRs,…

Solar and Stellar Astrophysics · Physics 2024-10-15 Zhuowen Li , Chunhua Zhu , Guoliang Lü , Lin Li , Helei Liu , Sufen Guo , Jinlong Yu , Xizhen Lu

In dwarf galaxies, nuclear star clusters (NSCs) are believed to primarily form from the migration and merger of globular clusters (GCs), with a possible contribution from in-situ star-forming activity triggered by gas infall. We present the…

(Abridged) We have performed a comprehensive multiwavelength analysis of a sample of 20 starburst galaxies that show the presence of a substantial population of massive stars. The main aims are the study of the massive star formation and…

Astrophysics · Physics 2011-08-31 Angel R. Lopez-Sanchez , Cesar Esteban

We have searched for dense molecular gas in three barred spiral galaxies with young starbursts, NGC 3049, 5430 and 6764, which are known Wolf-Rayet galaxies. We detected HCN in the latter two, and CS was marginally detected in NGC 6764. The…

Astrophysics · Physics 2007-05-23 T. Contini , H. Wozniak , S. Considere , E. Davoust

ISO-SWS spectroscopy of the WR galaxy NGC5253 is presented, and analysed to provide estimates of its hot young star population. Our approach differs from previous investigations in that we are able to distinguish between the regions in…

Though S0 galaxies are usually thought to be `red and dead', they demonstrate often star formation organized in ring structures. We try to clarify the nature of this phenomenon and its difference from star formation in spiral galaxies. The…

Astrophysics of Galaxies · Physics 2020-02-19 I. Proshina , O. Sil'chenko , A. Moiseev

In this work I communicate the detection of a new Galactic Wolf-Rayet star (WR60a) in Centaurus. The H- and K-band spectra of WR60a, show strong carbon near-infrared emission lines, characteristic of Wolf-Rayet stars of the WC5-7 sub-type.…

Astrophysics of Galaxies · Physics 2011-09-16 A. Roman-Lopes

The star-forming regions (SFRs) in the peculiar galaxies NGC 660, NGC 1512, NGC 4395 and NGC 4618 are studied. The relationships between such characteristics of star forming regions as UV, nearand far-IR fluxes, as well as in the Halpha and…

Astrophysics of Galaxies · Physics 2020-10-13 K. I. Smirnova , D. S. Wiebe , A. V. Moiseev , G. I. G. Józsa

We analyze longslit spectral observations of fourteen Wolf-Rayet galaxies from the sample of Schaerer, Contini & Pindao (1999). All 14 galaxies show broad Wolf-Rayet emission in the blue region of the spectrum, consisting of a blend of…

Astrophysics · Physics 2009-11-10 I. F. Fernandes , R. de Carvalho , T. Contini , R. R. Gal

We present measurements of stellar population properties of a newly discovered spectroscopically confirmed $z=11.10^{+0.11}_{-0.26}$, gravitationally lensed galaxy, using JWST NIRSpec PRISM spectroscopy and NIRCam imaging. The arc is highly…

Recent work has identified a population of low-redshift E/S0 galaxies that lie on the blue sequence in color vs. stellar mass parameter space, where spiral galaxies typically reside. While high-mass blue-sequence E/S0s often resemble young…

Cosmology and Nongalactic Astrophysics · Physics 2014-11-20 L. H. Wei , S. J. Kannappan , S. N. Vogel , A. J. Baker

We report the discovery of two new Wolf-Rayet (WR) galaxies: Mrk~1039, and F08208$+$2816. Two broad WR bumps at 5808\AA~ and 4650\AA~ indicate the presence of WCE and WNL star population in all two sources. We also confirm the presenceof WR…

Astrophysics · Physics 2009-10-30 J. H. Huang , Q. S. Gu , L. Ji , W. D. Li , J. Y. Wei , W. Zheng
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