中文
相关论文

相关论文: IC 10: More evidence that it is a blue compact dwa…

200 篇论文

We present near infrared JHK photometry for the central area of the irregular dwarf galaxy IC10. Comparing the red supergiants of IC10 and IC1613 we have determined the reddening of E(B-V)=1.05+-0.10 and the dereddened distance modulus…

天体物理学 · 物理学 2009-09-25 J. Borissova , L. Georgiev , M. Rosado , R. Kurtev , A. Bullejos , M. Valdez-Gutierrez

We estimate the reddening and distance of the nearest starburst galaxy IC 10 using deep near infrared $JHK_{S}$ photometry obtained with the Multi-Object InfraRed Camera and Spectrograph (MOIRCS) on the Subaru telescope. We estimate the…

宇宙学与河外天体物理 · 物理学 2015-05-13 Minsun Kim , Eunhyeuk Kim , Narae Hwang , Myung Gyoon Lee , Myungshin Im , Hiroshi Karoji , Junichi Noumaru , and Ichi Tanaka

The Local Group starburst galaxy IC10 is the closest example of a blue compact galaxy. Here, we use optical gi imaging from CFHT/MegaCam and near infra-red JHK imaging from UKIRT/WFCAM to conduct a comprehensive survey of the structure of…

星系天体物理 · 物理学 2015-10-07 Stephanie A. N. Gerbrandt , Alan W. McConnachie , Mike Irwin

IC 10 as a starburst dwarf galaxy in the Local Group (LG) has a large population of newly formed stars that are massive and intrinsically very bright in comparison with other LG galaxies. Using the Isaac Newton Telescope (INT) with the Wide…

星系天体物理 · 物理学 2023-06-12 Mahtab Gholami , Atefeh Javadi , Jacco Th. van Loon , Habib Khosroshahi , Elham Saremi

We have observed the Blue Compact Dwarf (BCD) galaxy He 2-10 in the 10 microns mid-infrared (MIR) atmospheric window using broad-band filters centered at lambda=10.1 microns and lambda=11.65 microns. In both filters, only the galaxy's…

天体物理学 · 物理学 2007-05-23 M. Sauvage , T. X. Thuan , P. O. Lagage

We present deep and accurate optical photometry of the Local Group starburst galaxy IC10. The photometry is based on two sets of images collected with the Advanced Camera for Surveys and with the Wide Field Planetary Camera 2 on board the…

We have measured the distance to the Local Group dwarf irregular galaxy IC 10 from near-infrared $JHK$ observations of Cepheids. The reddening-corrected distance modulus is $24.57\pm0.21$ mag or $0.82\pm 0.08$ Mpc. This distance lies at the…

天体物理学 · 物理学 2009-10-28 C. D. Wilson , D. L. Welch , I. N. Reid , A. Saha , J. Hoessel

Using deep 21-cm HI data from the Green Bank Telescope we have detected an ~18.3 kpc-long gaseous extension associated with the starbursting dwarf galaxy IC 10. The newly-found feature stretches 1.3 deg to the northwest and has a large…

We report the discovery of the first known symbiotic star in IC10, a starburst galaxy belonging to the Local Group, at a distance of ~750kpc. The symbiotic star was identified during a survey of emission-line objects. It shines at V =…

In this paper we analyze Very Large Array (VLA) telescope and Green Bank Telescope (GBT) atomic hydrogen (HI) data for the LITTLE THINGS(1) blue compact dwarf galaxy IC 10. The VLA data allow us to study the detailed HI kinematics and…

HI observations of the nearby blue compact dwarf galaxy IC 10 obtained with the Dominion Radio Astrophysical Observatory synthesis telescope (DRAO), for a total integration of $\sim$1000 hours, are presented. We confirm the NW faint 21 cm…

星系天体物理 · 物理学 2020-01-08 Brenda Namumba , Claude Carignan , Tyler Foster , Nathan Deg

We present submillimeter observations of the Local Group, metal-poor, irregular dwarf galaxy IC 10, directly relevant to the interaction between interstellar medium and star formation activity in primeval galaxies. Using the JCMT, we have…

We present new deep and accurate space (Advanced Camera for Surveys -- Wide Field Planetary Camera 2 at the Hubble Space Telescope) and ground-based (Suprime-Cam at Subaru Telescope, Mega-Cam at Canada-France-Hawaii Telescope) photometric…

We study the evolved stellar population of the Local Group galaxy IC10, with the aim of characterizing the individual sources observed and to derive global information on the galaxy, primarily the star formation history and the dust…

太阳与恒星天体物理 · 物理学 2018-07-04 F. Dell'Agli , M. Di Criscienzo , P. Ventura , M. Limongi , D. A. García--Hernández , E. Marini , C. Rossi

We report the detection of oxygen-rich circumstellar envelopes in stars of the nearby (700 kpc) starburst galaxy IC 10. The star formation history and the chemical environment of this galaxy makes it an ideal target to observe dust…

太阳与恒星天体物理 · 物理学 2015-06-11 V. Lebouteiller , G. C. Sloan , M. A. T. Groenewegen , M. Matsuura , D. Riebel , D. G. Whelan , J. Bernard-Salas , P. Massey , E. Bayet

In young starburst galaxies, the X-ray population is expected to be dominated by the relics of the most massive and short-lived stars, black-hole and neutron-star high mass X-ray binaries (XRBs). In the closest such galaxy, IC 10, we have…

高能天体物理现象 · 物理学 2017-02-15 Silas G. T. Laycock , Dimitris M. Christodoulou , Benjamin F. Williams , Breanna Binder , Andrea Prestwich

IC 10 is the nearest starburst irregular galaxy remarkable for its anomalously high number of WR stars. We report the results of an analysis of the emission spectra of HII-regions ionized by star clusters and WR stars based on observations…

宇宙学与河外天体物理 · 物理学 2015-05-19 O. V. Egorov , V. P. Arkhipova , T. A. Lozinskaya , A. V. Moiseev

IC10 is the nearest starburst galaxy, as revealed both by its Halpha surface brightness and the large number of Wolf-Rayet stars (WRs) per unit area. The relative number of known WC- to WN-type WRs has been thought to be unusually high…

天体物理学 · 物理学 2009-11-07 Philip Massey , Shadrian Holmes

We present an analysis of $\sim$235 ks of Chandra observations obtained over $\sim$19 years of the nearby dwarf starburst galaxy IC 10 in order to study the X-ray variability and X-ray luminosity function (XLF) of its X-ray binary (XRB)…

高能天体物理现象 · 物理学 2025-08-06 Breanna A. Binder , Rosalie Lazarus , Mina Thoresen , Silas Laycock , Sayantan Bhattacharya

We report the results of spectroscopic observations, obtained with the Gemini North Multi-Object Spectrograph, of 9 planetary nebulae (PNe) and 15 \hii\ regions located in the 5.5\arcmin $\times$5.5\arcmin inner region of the nearby…

宇宙学与河外天体物理 · 物理学 2015-05-13 Laura Magrini , Denise R. Goncalves
‹ 上一页 1 2 3 10 下一页 ›