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相关论文: PGC 44685: A Dwarf Star-forming Lenticular Galaxy …

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Lenticular galaxies (S0s) were considered mainly as passive evolved spirals due to environmental effects for a long time; however, most S0s in the field cannot fit into this common scenario. In this work, we study one special case, SDSS…

星系天体物理 · 物理学 2021-07-07 Zhengyi Chen , Qiu-Sheng Gu , Rubén García-Benito , Zhi-Yu Zhang , Xue Ge , Mengyuan Xiao , Xiaoling Yu

Lenticular galaxies (S0s) in the local universe are generally absent of recent star formation and lack molecular gas. In this paper, we investigate one massive ($M_*$$\sim$5$\times10^{10}$ M$_\odot$) star-forming S0, PGC 39535, with the…

星系天体物理 · 物理学 2024-09-10 Jiantong Cui , Qiusheng Gu , Shiying Lu , Zhengyi Chen , Can Xu , Zeyu Gao

We present here spatially-resolved optical spectroscopic observations of four nearby dwarf Wolf-Rayet (WR) galaxies. The ages of the most recent starburst events in these galaxies are found between 3 and 10 Myr. The gas-phase metallicities…

星系天体物理 · 物理学 2018-10-31 A. Paswan , A. Omar , S. Jaiswal

Very little work has been done on star formation in dwarf lenticular galaxies (S0s). We present 2D-spectroscopic and millimetre observations made by Centro Astronomico Hispano Aleman (CAHA) 3.5 m optical and the IRAM-30 m millimetre…

星系天体物理 · 物理学 2021-09-22 Xue Ge , Qiu-Sheng Gu , Ruben Garcıa-Benito , Shi-Ying Lu , Cheng-Long Lei , Nan Ding

It is widely believed that lenticular (S0) galaxies were initially spirals from which the gas has been removed by interactions with hot cluster gas, or by ram-pressure stripping of cool gas from spirals that are orbiting within rich…

宇宙学与河外天体物理 · 物理学 2015-05-13 Sidney van den Bergh

Comparing to the inactive and gas-poor normal lenticular galaxies (S0s) in the local universe, we study a barred star-forming S0 galaxy, PGC 34107, which has been observed by the Centro Astron\'{o}mico Hispano Alem\'{a}n (CAHA) 3.5-m…

星系天体物理 · 物理学 2022-03-30 Shiying Lu , Qiusheng Gu , Xue Ge , Luis C. Ho , Yulong Gao , Zhengyi Chen , Ke Xu , Zhi-Yu Zhang , Yong Shi , Qirong Yuan , Min Bao

As one type of blue early-type galaxies, the evolutionary history and fate of star-forming lenticular galaxies (S0s) remain elusive. We selected 134 star-forming S0s from the SDSS-IV MaNGA survey and found that they have steep and warped…

星系天体物理 · 物理学 2024-12-20 Pei-Bin Chen , Junfeng Wang , Tian-Wen Cao , Mengting Shen , Xiaoyu Xu

Aims: We investigate the massive stellar content of the nearby dwarf irregular Wolf-Rayet galaxy IC 4662, and consider its global star forming properties in the context of other metal-poor galaxies, the SMC, IC 10 and NGC 1569. Methods:…

宇宙学与河外天体物理 · 物理学 2015-05-13 P. A. Crowther , J. L. Bibby

Lenticular galaxies are generally thought to have descended from spirals via morphological transformation, although recent numerical simulations have shown that minor or even major merger can also lead to an S0-like remnant. These…

星系天体物理 · 物理学 2018-08-08 Kanak Saha , Arianna Cortesi

We present a study of the properties of star-forming regions within a sample of 7 Wolf-Rayet (WR) galaxies. We analyze their morphologies, colours, star-formation rate (SFR), metallicities, and stellar populations combining broad-band and…

宇宙学与河外天体物理 · 物理学 2013-12-02 Chrisphin Karthick. M , Angel R. Lopez-Sanchez , D. K. Sahu , B. B. Sanwal , Shuchi Bisht

Wolf-Rayet (WR) galaxies are a rare population of galaxies that host living high-mass stars during their WR phase (i.e. WR stars) and are thus expected to provide interesting constraints on the stellar Initial Mass Function, massive star…

星系天体物理 · 物理学 2020-07-01 Fu-Heng Liang , Cheng Li , Niu Li , Renbin Yan , Houjun Mo , Wei Zhang , Camilo Machuca , Alexandre Roman-Lopes

Star formation histories (SFHs) are essential for understanding galaxy formation and evolution. We present the mean SFHs of 148 dwarf lenticular galaxies (dS0s) derived from the Sloan Digital Sky Survey (SDSS) spectra. These SFHs reveal two…

星系天体物理 · 物理学 2024-03-29 Hong Bae Ann , Mira Seo

Despite numerous efforts, it is still unclear whether lenticular galaxies (S0s) evolve from spirals whose star formation was suppressed, or formed trough mergers or disk instabilities. In this paper we present a pilot study of 21 S0…

We test the theory that lenticular (S0) galaxies form from spirals whose star formation has been shut down. We use the globular cluster specific frequency S_N, defined as the number of globular clusters normalised by the galaxy luminosity…

天体物理学 · 物理学 2009-11-13 J. M. Barr , A. G. Bedregal , A. Aragon-Salamanca , M. R. Merrifield , S. P. Bamford

Though S0 galaxies are usually thought to be `red and dead', they often demonstrate weak star formation organised in ring structures and located in their outer disks. We try to clarify the nature of this phenomenon and its difference from…

星系天体物理 · 物理学 2023-01-18 O. Sil'chenko , A. Moiseev , D. Oparin , J. E. Beckman , J. Font

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…

星系天体物理 · 物理学 2019-06-19 Irina S. Proshina , Alexei Yu. Kniazev , Olga K. Sil'chenko

Nearby metal-poor starburst dwarf galaxies present a unique opportunity to probe the physics of high-density star formation with a detail and sensitivity unmatched by any observation of the high-z Universe. Here we present the first results…

Lenticular (S0) galaxies are galaxies that exhibit a bulge and disk component, yet lack any clear spiral features. With features considered intermediary between spirals and ellipticals, S0s have been proposed to be a transitional…

星系天体物理 · 物理学 2023-03-02 Mitchell K. Cavanagh , Kenji Bekki , Brent A. Groves

We report the first-ever discovery of a Wolf-Rayet (WR) star in the Large Magellanic Cloud via detection of a circular shell with the Spitzer Space Telescope. Follow-up observations with Gemini-South resolved the central star of the shell…

太阳与恒星天体物理 · 物理学 2015-06-19 V. V. Gvaramadze , A. -N. Chene , A. Y. Kniazev , O. Schnurr , T. Shenar , A. Sander , R. Hainich , N. Langer , W. -R. Hamann , Y. -H. Chu , R. A. Gruendl

(Abridged) We have performed a comprehensive multiwavelength analysis of a sample of 20 starburst galaxies that show the presence of a substantial population of very young massive stars. In this paper, the second of the series, we present…

宇宙学与河外天体物理 · 物理学 2015-05-14 Angel R. Lopez-Sanchez , Cesar Esteban
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