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Related papers: Outlying H$\alpha$ blobs in SDSS IV MaNGA

200 papers

We report the discovery of 854 ultra diffuse galaxies (UDGs) in the Coma cluster using deep R band images, with partial B, i, and Halpha band coverage, obtained with the Subaru telescope. Many of them (332) are Milky Way-sized with very…

Astrophysics of Galaxies · Physics 2015-06-08 Jin Koda , Masafumi Yagi , Hitomi Yamanoi , Yutaka Komiyama

We study the heating mechanisms and Ly{\alpha} escape fractions of 35 Ly{\alpha} blobs (LABs) at z = 3.1 in the SSA22 field. Dust continuum sources have been identified in 11 of the 35 LABs, all with star formation rates (SFRs) above 100…

Recent VLA observations pointed at dwarf spheroidal (dSph) galaxies in the M 81 group reveal a hitherto hidden population of extremely low mass (~1e5 Msol) HI clouds with no obvious optical counterparts. We have searched 10 fields in the…

Astrophysics · Physics 2009-11-13 Elias Brinks , Fabian Walter , Evan D. Skillman

The results of an Halpha photometric survey of 30 dwarf galaxies of various morphologies in the Centaurus A and Sculptor groups are presented. Of these 30, emission was detected in 13: eight are of late-type, two are early-type and three…

Astrophysics · Physics 2009-11-13 A. Bouchard , G. S. Da Costa , H. Jerjen

By applying spectroscopic decomposition methods to a sample of MaNGA early-type galaxies, we separate out spatially and kinematically distinct stellar populations, allowing us to explore the similarities and differences between galaxy…

Owing to their quiet evolutionary histories, nearby dwarf galaxies (stellar masses $M_\star \lesssim 3 \times 10^9 M_\odot$) have the potential to teach us about the mechanism(s) that 'seeded' the growth of supermassive black holes, and…

We update our stellar population models for the time evolution of the number and mass of massive remnants - neutron stars and black holes - with a new initial mass-remnant mass relation for core collapse supernovae. The calculations are…

Precise abundance ratios are determined for 94 dwarf stars with 5200 < Teff < 6300 K, -1.6 < [Fe/H] < -0.4, and distances D < 335 pc. Most of them have halo kinematics, but 16 thick-disk stars are included. Equivalent widths of atomic lines…

Astrophysics of Galaxies · Physics 2015-05-18 Poul E. Nissen , William J. Schuster

We study 379 central and 159 satellite early-type galaxies with two-dimensional kinematics from the integral-field survey Mapping Nearby Galaxies at APO (MaNGA) to determine how their angular momentum content depends on stellar and halo…

We investigate the origin of rare star-formation in an otherwise red-and-dead population of S0 galaxies using spatially resolved spectroscopy. Our sample consists of $120$ low redshift ($z<0.1$) star-forming S0 (SF-S0) galaxies from the…

Astrophysics of Galaxies · Physics 2022-04-06 Himansh Rathore , Kavin Kumar , Preetish K. Mishra , Yogesh Wadadekar , Omkar Bait

We present optical photometry of Hubble Space Telescope (HST) ACS/WFC data of the resolved stellar populations in the outer disc of the dwarf irregular galaxy DDO 154. The photometry reveals that young main sequence stars are almost absent…

Astrophysics of Galaxies · Physics 2018-05-02 Adam B. Watts , Gerhardt R. Meurer , Claudia D. P. Lagos , Sarah M. Bruzzese , Pavel Kroupa , Tereza Jerabkova

Dwarf novae in globular clusters seem to be rare with only 13 detections in the 157 known Galactic globular clusters. We report the identification of a new dwarf nova in M13, the 14th dwarf nova identified in a globular cluster to date.…

Solar and Stellar Astrophysics · Physics 2015-05-27 Mathieu Servillat , N. A. Webb , F. Lewis , C. Knigge , M. van den Berg , A. Dieball , J. Grindlay

We have used the VIMOS integral field spectrograph to map the emission line properties in a sample of 24 star forming galaxies selected from the SDSS database. In this data paper we present and describe the sample, and explore some basic…

Cosmology and Nongalactic Astrophysics · Physics 2015-06-03 J. Gerssen , D. J. Wilman , L. Christensen

This paper reports follow-up photometric and spectroscopic observations, including warm Spitzer IRAC photometry of seven white dwarfs from the SDSS with apparent excess flux in UKIDSS K-band observations. Six of the science targets were…

Solar and Stellar Astrophysics · Physics 2012-06-06 J. Farihi , B. T. Gänsicke , P. R. Steele , J. Girven , M. R. Burleigh , E. Breedt , D. Koester

We analyse two-dimensional maps and radial profiles of EW(H$\alpha$), EW(H$\delta_A$), and D$_n$(4000) of low-redshift galaxies using integral field spectroscopy from the MaNGA survey. Out of $\approx1400$ nearly face-on late-type galaxies…

Astrophysics of Galaxies · Physics 2020-09-30 Lin Lin , Cheng Li , Cheng Du , Enci Wang , Ting Xiao , Martin Bureau , Amelia Fraser-McKelvie , Karen Masters , Lihwai Lin , David Wake , Lei Hao

We present a sample of 17 objects from the CALIFA survey where we find initial evidence of galactic winds based on their off-axis ionization properties. We identify the presence of outflows using various optical diagnostic diagrams (e.g.,…

Galactic outflows are predicted to be ubiquitous in low-mass galaxies, but observational evidence is lacking. Both a low signal-to-noise and a low spectral resolution can severely hamper the detection of galactic outflows, especially in…

Astrophysics of Galaxies · Physics 2026-05-27 B. Hagedorn , C. Cicone , C. Vignali , P. Severgnini , M. Pedani , M. Sarzi , A. Saintonge , M. Romano

We present a general phenomenological model for the metallicity distribution (MD) in terms of [Fe/H] for dwarf spheroidal galaxies (dSphs). These galaxies appear to have stopped accreting gas from the intergalactic medium and are fossilized…

Astrophysics of Galaxies · Physics 2015-06-04 Yong-Zhong Qian , Gerald J. Wasserburg

We measure $\lambda_{R_e}$, a proxy for galaxy specific stellar angular momentum within one effective radius, and the ellipticity, $\epsilon$, for about 2300 galaxies of all morphological types observed with integral field spectroscopy as…

HST spectroscopical observations of 8 HII galaxies are reported. Ly alpha emission was detected in 4 of them. We find that the velocity structure of the gas is the main determining factor for the escape of the Ly alpha photons, and not the…

Astrophysics · Physics 2007-05-23 D. Kunth , J. Lequeux , J. M. Mas-Hesse , E. Terlevich , R. Terlevich