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Related papers: Uncovering Blue Diffuse Dwarf Galaxies

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X-rays from binaries in small, metal-deficient galaxies may have contributed significantly to the heating and reionization of the early universe. We investigate this claim by studying blue compact dwarfs (BCDs) as local analogues to these…

Astrophysics of Galaxies · Physics 2015-06-19 Matthew Brorby , Philip Kaaret , Andrea Prestwich

We present a sample of hard X-ray selected candidate black holes (BHs) in 19 dwarf galaxies. BH candidates are identified by cross-matching a parent sample of ~44,000 local dwarf galaxies (M_stellar < 3 x 10^9 Msun, z<0.055) with the…

Astrophysics of Galaxies · Physics 2015-05-27 Sean Lemons , Amy Reines , Richard Plotkin , Elena Gallo , Jenny Greene

We present 6.5-meter MMT and 3.5m APO spectrophotometry of 69 H II regions in 42 low-metallicity emission-line galaxies, selected from the Data Release 7 of the Sloan Digital Sky Survey to have mostly [O III]4959/Hbeta < 1 and [N…

Cosmology and Nongalactic Astrophysics · Physics 2018-05-29 Y. I. Izotov , T. X. Thuan , N. G. Guseva

We present a {\em Spitzer}-based mid-infrared study of a large sample of Blue Compact Dwarf galaxies (BCD) using the Infrared Spectrograph (IRS), including the first mid-IR spectrum of IZw18, the archetype for the BCD class and among the…

We present a re-analysis of spectroscopic data for 23 HII-regions in 12 blue, metal-poor low surface brightness galaxies (LSBGs) taking advantage of recent developments in calibrating strong-line methods. In doing so we have identified a…

Cosmology and Nongalactic Astrophysics · Physics 2015-03-19 Lars Mattsson , Leonid S. Pilyugin , Nils Bergvall

Dwarf galaxies play an important role in our understanding of galaxy formation and evolution, and starbursts are believed to strongly affect their structure and evolution. Here we present a study of 12 of the nearest dwarf galaxies thought…

Astrophysics · Physics 2009-10-31 Amanda T. Marlowe , Gerhardt R. Meurer , Timothy M. Heckman

We present spectroscopic observations of the nearby dwarf galaxy AGC 198691. This object is part of the Survey of HI in Extremely Low-Mass Dwarfs (SHIELD) project, which is a multi-wavelength study of galaxies with HI masses in the range of…

We present 6.5-meter MMT spectrophotometry of 20 H II regions in 13 extremely metal-poor emission-line galaxies selected from the Data Release 5 of the Sloan Digital Sky Survey to have [O III] 4959/Hbeta < 1 and [N II] 6583/Hbeta < 0.05.…

Astrophysics · Physics 2009-11-13 Y. I. Izotov , T. X. Thuan

(abridged) We present deep archival VLT/FORS1+UVES spectroscopic observations of the system of two blue compact dwarf (BCD) galaxies SBS 0335-052E and SBS 0335-052W. Our aim is to derive element abundances in different HII regions of this…

Cosmology and Nongalactic Astrophysics · Physics 2018-05-30 Y. I. Izotov , N. G. Guseva , K. J. Fricke , P. Papaderos

Extremely metal-poor stars are intrinsically rare, but emerging methods exist to accurately classify them from all-sky Gaia XP low-resolution spectra. To assess their overall accuracy for targeting metal-poor stars, we present a…

Solar and Stellar Astrophysics · Physics 2026-01-30 Riley Thai , Andrew R. Casey , Alexander Ji , Vedant Chandra , Hans-Walter Rix

It has long been speculated that Blue Compact Dwarf galaxies (BCDs) are formed through the interaction between low-mass gas-rich galaxies, but a few candidates of such systems have been studied in detail. We study a sample of compact…

Astrophysics of Galaxies · Physics 2022-12-15 Daya Nidhi Chhatkuli , Sanjaya Paudel , Rajesh Kumar Bachchan , Binil Aryal , Jaewon Yoo

We report the discovery of a rare isolated group of five dwarf galaxies located at z = 0.0086 ($D$ = 36 Mpc). All member galaxies are star-forming, blue, and gas-rich with $g-r$ indices ranging from 0.2 to 0.6 mag, and two of them show…

Astrophysics of Galaxies · Physics 2024-11-18 Sanjaya Paudel , Cristiano G. Sabiu , Suk-Jin Yoon , Pierre-Alain Duc , Jaewon Yoo , Oliver Müller

Blue early-type galaxies with galaxy-scale ongoing star formation are interesting targets in order to understand the stellar mass buildup in elliptical and S0 galaxies in the local Universe. We study the star-forming population of blue…

Astrophysics of Galaxies · Physics 2023-09-27 Koshy George

Blue metal-poor stars are main-sequence stars that are bluer and brighter than typical turn-off stars in metal-poor globular clusters. They are thought to have either evolved through post-mass transfer mechanisms as field blue straggler…

We used the $H\alpha$ images from a large sample of nearby late-type dwarf galaxies to investigate properties of their emission structure. The sample consists of three hundred galaxies of the irregular (Irr), Magellanic irregular (Im), blue…

Astrophysics of Galaxies · Physics 2020-12-16 Karachentsev I. D. , Kaisin S. S

In this paper, we report our studies on the gaseous and chemical properties of a relatively large sample (53 members) of blue compact dwarf galaxies (BCDs). The results of correlations among the oxygen abundance, stellar mass, gas mass,…

Cosmology and Nongalactic Astrophysics · Physics 2013-01-28 Yinghe Zhao , Yu Gao , Qiusheng Gu

We present a sample of 48 metal-poor galaxies at $ z < 0.14$ selected from 92,510 galaxies in the LAMOST survey. These galaxies are identified for their detection of the auroral emission line \oiii$\lambda$4363 above $3\sigma$ level, which…

Astrophysics of Galaxies · Physics 2017-05-10 Yulong Gao , Jianhui Lian , Xu Kong , Zesen Lin , Ning Hu , Haiyang Liu , Enci Wang , Zihuang Cao , Yonghui Hou , Yuefei Wang , Yong Zhang

We present photometric and spectroscopic observations of two luminous blue variable (LBV) stars in two extremely metal-deficient blue compact dwarf (BCD) galaxies, DDO 68 with 12+logO/H = 7.15 and PHL 293B with 12+logO/H = 7.72. These two…

Astrophysics · Physics 2014-11-18 Y. I. Izotov , T. X. Thuan

We present long slit optical spectroscopy of 67 HII regions in 21 dwarf irregular galaxies to investigate the enrichment of oxygen, nitrogen, neon, sulfur, and argon in low mass galaxies. Oxygen abundances are obtained via direct detection…

Astrophysics · Physics 2009-11-13 L. van Zee , M. P. Haynes

Untargeted neutral hydrogen (HI) surveys are well suited to identifying low surface brightness galaxies (LSBGs) that are gas rich, and they offer a complementary view to optically selected populations. We examined the LSBG population as…

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