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Related papers: IC 10: More evidence that it is a blue compact dwa…

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We present the spectroscopic discovery of a broad-lined Type Ic supernova (SN 2010bh) associated with the nearby long-duration gamma-ray burst (GRB) 100316D. At z = 0.0593, this is the third-nearest GRB-SN. Nightly optical spectra obtained…

We present Spitzer imaging of the metal-deficient (Z ~30% Z_sun) Local Group dwarf galaxy NGC 6822. On spatial scales of ~130 pc, we study the nature of IR, H alpha, HI, and radio continuum emission. Nebular emission strength correlates…

We investigate the star formation history of the central regions of four Luminous Compact Blue Galaxies (LCBGs). LCBGs are blue (B-V<0.6), compact (MU_B<21.5 mag arcsec^-2) galaxies with absolute magnitudes M_B brighter than -17.5. The…

Astrophysics · Physics 2008-11-26 C. Hoyos , R. Guzman , A. I. Diaz , D. C. Koo , M. A. Bershady , .

Mid-infrared spectra from the Medium Resolution Spectrometer on the James Webb Space Telescope have revealed the molecular chemistry of carbon stars in the Large Magellanic Cloud with better resolution and sensitivity than previously…

We present measurements of the 3.4-micron hydrocarbon dust absorption feature, and four visual diffuse interstellar bands, for twelve highly reddened (9.0<A(V)<15.8), early-type stars identified from the Stephenson (1992) catalogue,…

Astrophysics · Physics 2009-11-07 M. G. Rawlings , A. J. Adamson , D. C. B. Whittet

A sample of 34 dwarf irregular galaxies in the Local Volume, most nearer than 5 Mpc, has been imaged in the near-infrared (NIR) in J and K_s at CFHT in Hawaii and OAN-SPM in Mexico. In CFHT images, stars brighter than M_Ks=-7.5 were…

Astrophysics · Physics 2009-09-29 Ovidiu Vaduvescu , Marshall L. McCall , Michael G. Richer , Robin L. Fingerhut

IC 3418 is a dwarf irregular galaxy falling into the Virgo cluster, and a 17 kpc long trail is seen behind the galaxy, which is considered to have formed due to ram pressure stripping. The trail contains compact knots and diffuse blobs of…

Cosmology and Nongalactic Astrophysics · Physics 2013-04-10 Youichi Ohyama , Ananda Hota

The near and mid-infrared characteristics of large amplitude, Mira, variables in Local Group dwarf irregular galaxies (LMC, NGC 6822, IC 1613, Sgr dIG) are described. Two aspects of these variables are discussed. First, the short period (P…

Astrophysics of Galaxies · Physics 2017-11-27 Patricia A. Whitelock

We present a high spatial resolution CCD surface photometry study in the optical V, R and I broadband filters of a sample of 15 HII galaxies. The colours of the starburst continuum and of the underlying galaxy are measured. The distribution…

Astrophysics · Physics 2015-06-24 Eduardo Telles , Roberto Terlevich

We present the results of observations of the Irr galaxy IC 10 at the 6-m SAO telescope with the panoramic Multi-Pupil Fiber Spectrograph (MPFS). Based on the results of these observations and our long-slit spectroscopy performed…

Cosmology and Nongalactic Astrophysics · Physics 2011-07-15 V. P. Arkhipova , O. V. Egorov , T. A. Lozinskaya , A. V. Moiseev

Near- and mid-IR survey data from DENIS and ISOGAL are used to investigate the structure and formation history of the inner 10 degree (1.4 kpc) of the Milky Way galaxy. Synthetic bolometric corrections and extinction coefficients in the…

Optical spectroscopy of the blue star KIC 10449976 shows that it is an extremely helium-rich subdwarf with effective temperature T=40000+/-300 K and surface gravity log g=5.3+/-0.1. Radial-velocity measurements over a five-day timescale…

Solar and Stellar Astrophysics · Physics 2015-06-12 C. S. Jeffery , G. Ramsay , N. Naslim , R. Carrera , S. Greiss , T. Barclay , R. Karjalainen , A. Brooks , P. Hakala

ISOCAM extragalactic mid-infrared deep surveys have detected a population of strong IR emitters ten times more numerous than expected if there were no evolution from z<0.2 (IRAS) up to the maximum redshift of these galaxies (z=1.5). The…

We present the discovery of a peculiar blue core in the elliptical galaxy IC 225 by using images and spectrum from the Sloan Digital Sky Survey (SDSS). The outer parts of the surface brightness profiles of u-, g-, r-, i- and z-band SDSS…

Astrophysics · Physics 2008-11-26 Qiusheng Gu , Yinghe Zhao , Lei Shi , Zhixin Peng , Xinlian Luo

We present deep $BVI$ observations of the dwarf irregular galaxy UKS1927-177 in Sagittarius. Statistically cleaned $V$, $(B-I)$ CMDs clearly display the key evolutionary features in this galaxy. Previously detected C stars are located in…

Astrophysics · Physics 2009-11-07 Y. Momany , E. V. Held , I. Saviane , L. Rizzi

We present a pilot study on the origin and assembly history of the ICL for four galaxy clusters at 0.44<z<0.57 observed with the Hubble Space Telescope from the Cluster Lensing and Supernova Survey with Hubble (CLASH) sample. Using this…

Astrophysics of Galaxies · Physics 2015-06-23 Tahlia DeMaio , Anthony Gonzalez , Ann Zabludoff , Dennis Zaritsky , Marusa Bradac

We present Spitzer observations of the blue compact dwarf galaxy (BCD) Haro 3, with an oxygen abundance of 12+log(O/H)=8.32. These data are part of a larger study of star formation and dust in low-metallicity environments.The IRS spectrum…

Astrophysics · Physics 2008-11-26 L. K. Hunt , T. X. Thuan , M. Sauvage , Y. I. Izotov

A CO(1-0) on-source spectrum of the well-known carbon star IRC+10216 taken with the IRAM 30m telescope in June 1996 shows excess emission between -18.3 and -14.3 km/s at the red wing of the underlying profile. The excess emission is…

Astrophysics · Physics 2009-09-25 M. A. T. Groenewegen , H. -G. Ludwig

Spitzer Space Observatory IRAC and MIPS photometric observations are presented for 20 white dwarfs with T < 20,000 K and metal-contaminated photospheres. A warm circumstellar disk is detected at GD 16 and likely at PG 1457-086, while the…

Earth and Planetary Astrophysics · Physics 2011-02-11 J. Farihi , M. Jura , B. Zuckerman

We observed an area of 10 deg^2 of the Large Magellanic Cloud using the Infrared Camera on board AKARI. The observations were carried out using five imaging filters (3, 7, 11, 15, and 24 micron) and a dispersion prism (2 -- 5 micron,…