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The formation of pillars of dense gas at the boundaries of H II Regions is investigated with hydrodynamical numerical simulations including ionising radiation from a point source. We show that shadowing of ionising radiation by an…

星系天体物理 · 物理学 2014-11-20 Jonathan Mackey , Andrew J. Lim

The formation and evolution of elliptical galaxies (EGs) is still an open question. In particular, recent observations suggest that elliptical galaxies are not only simple spheroidal systems of old stars. In this paper we analyze a sample…

星系天体物理 · 物理学 2013-04-09 Song Huang , Qiu-Sheng Gu

The ~70 unidentified sources of the EGRET sky survey may be one of its most important legacies. The identification of these sources at other wavelengths is critical to understanding their nature. Many have flat spectra out to 10 GeV which,…

We present a stellar population analysis of quiescent (without H$\alpha$ emission) and bright ($M_{r}$ $<$ $-$21.5) early-type galaxies (ETGs) with recent star formation. The ETGs are selected from a spectroscopic sample of SDSS galaxies at…

星系天体物理 · 物理学 2016-04-13 Jongwan Ko , Haeun Chung , Ho Seong Hwang , Jong Chul Lee

We present near-IR spectroscopy of three Extremely Red Objects (EROs) using the OHS/CISCO spectrograph at Subaru telescope. One target exhibits a strong emission line which we identify as H-alpha at z = 1.34. Using new and existing…

天体物理学 · 物理学 2009-11-10 Garret Cotter , Chris Simpson , Rosemary C. Bolton

The HII region IC 1848 harbors a lot of intricate elephant trunk-like structures that look morphologically different from usual bright-rimmed clouds (BRCs). Of particular interest is a concentration of thin and long elephant trunk-like…

太阳与恒星天体物理 · 物理学 2015-05-28 Neelam Chauhan , Katsuo Ogura , Anil K. Pandey , Manash R. Samal , Bhuwan C. Bhatt

Massive SFR are characterized by intense ionizing fluxes, strong stellar winds and supernovae explosions, all of which have important effects on the surrounding media, on the star-formation (SF) process and on the evolution of YSOs and…

太阳与恒星天体物理 · 物理学 2015-05-19 M. G. Guarcello , G. Micela , G. Peres , L. Prisinzano , S. Sciortino

Attention is given to a population of 110 stars in the NGC 6611 cluster of the Eagle Nebula that have prominent near-infrared (NIR) excess and optical colours typical of pre-main sequence (PMS) stars older than 8 Myr. At least half of those…

太阳与恒星天体物理 · 物理学 2015-06-16 Guido De Marchi , Nino Panagia , M. G. Guarcello , Rosaria Bonito

We present the results of near-infrared imaging simulations of young star-forming regions in the Magellanic Clouds to be observed with the European Extremely Large Telescope (E-ELT). The simulated J,H,K-band images show that we should be…

太阳与恒星天体物理 · 物理学 2011-09-29 Annalisa Calamida , Fernando Comeron , Hans Zinnecker

Dust in Early-Type galaxies (ETGs) may originate from internal or external sources. In this paper we study the stellar populations of particularly dusty ETGs to search for evidence of the dust's origin. Using the Southern African Large…

星系天体物理 · 物理学 2026-04-08 Ron W. Savage , Anne E. Sansom , David H. W. Glass

We measure oxygen and nitrogen abundances for 14 star-forming emission line galaxies (ELGs) at 0.11<z<0.5 using Keck/LRIS optical spectroscopy. The targets exhibit a range of metallicities from slightly metal-poor like the LMC to…

天体物理学 · 物理学 2009-10-30 Henry A. Kobulnicky , Dennis Zaritsky

We investigate the star formation occurring in a region well below the Galactic plane towards the optical reflection nebula ESO 368-8 (IRAS 07383-3325). We confirm the presence of a small young stellar cluster (or aggregate of tens of YSOs)…

星系天体物理 · 物理学 2015-05-14 Pedro M. Palmeirim , Joao L. Yun

NGC 1316 is a giant, elliptical galaxy containing a complex network of dark, dust features. The morphology of these features has been examined in some detail using a Hubble Space Telescope, Advanced Camera for Surveys image. It is found…

星系天体物理 · 物理学 2010-03-31 Per Carlqvist

Valuable insights into galaxy evolution can be gleaned from studies of resolved stellar populations in the local Universe. Deep photometric surveys have provided tracers of the star-formation histories in galaxies from 0.8-16 Mpc, but…

M16, the Eagle Nebula, is an outstanding HII region where extensive high-mass star formation is taking place in the Sagittarius Arm, and hosts the remarkable "pillars" observed with HST. We made new CO observations of the region in the 12CO…

The Rosette Nebula is an HII region ionized mainly by the stellar cluster NGC 2244. Elephant trunks, globules, and globulettes are seen at the interface where the HII region and the surrounding molecular shell meet. We have observed a field…

星系天体物理 · 物理学 2017-09-20 M. M. Mäkelä , L. K. Haikala , G. F. Gahm

We report on the neutral hydrogen gas content (21-cm emission) of eight extremely isolated early-type galaxies (IEGs) using the Green Bank Telescope. Emission is detected in seven of the eight objects. This paper is the third in a series…

星系天体物理 · 物理学 2019-04-10 Trisha Ashley , Pamela M. Marcum , Mehmet Alpaslan , Michael N. Fanelli , James D. Frost

We reconstruct the SFHs of 7 massive ($M_{\star}\gtrsim 10^{10} M_{\odot}$) early-type galaxies (ETGs) in the Virgo cluster by analysing their spatially resolved stellar population (SP), including their UV and H$\alpha$ emission. As part of…

We present a comprehensive analysis of dense cores and filamentary structures in the M16 Eagle Nebula using high-resolution ($11.7^{\prime\prime}$) surface density and temperature maps derived from \textit{Herschel} observations. Using the…

星系天体物理 · 物理学 2026-05-01 Nageen Pervaiz , Guo-Yin Zhang , Alexander Men'shchikov , Jin-Zeng Li