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(Abridged) We present a study of the ionizing stars associated with the diffuse ionized gas (DIG) and HII regions in the nearby spiral galaxy M33. We compare our Schmidt H-alpha image to the far-ultraviolet (FUV, 1520A) image from the…

天体物理学 · 物理学 2009-10-31 Charles G. Hoopes , Rene A. M. Walterbos

(Abridged) We have compared H-alpha and far ultraviolet (FUV) images of 10 nearby spirals, with the goal of understanding the contribution of field OB stars to the ionization of the diffuse ionized gas (DIG) in spiral galaxies. The FUV…

天体物理学 · 物理学 2009-11-06 Charles G. Hoopes , Rene A. M. Walterbos , Gregory D. Bothun

We compare Far-UV, H-alpha, and optical broadband images of the nearby spiral galaxy M33, to investigate the massive stars associated with the diffuse ionized gas. The H-alpha/FUV ratio is higher in HII regions than in the DIG, possibly…

天体物理学 · 物理学 2009-10-30 Charles G. Hoopes , Rene A. M. Walterbos

As part of a large study to map the distribution of star formation across galactic disks, we have obtained deep Halpha images of the nearby Sculptor Group spirals NGC 247 and NGC 7793. These images are of sufficiently high quality that they…

天体物理学 · 物理学 2007-05-23 Annette M. N. Ferguson , Rosemary F. G. Wyse , J. S. Gallagher , Deidre A. Hunter

We present a multiwavelength study of star formation within the nearby M101 Group, including new deep H$\alpha$ imaging of M101 and its two companions. We perform a statistical analysis of the H$\alpha$ to FUV flux ratios in HII regions…

星系天体物理 · 物理学 2017-12-27 Aaron E. Watkins , J. Christopher Mihos , Paul Harding

We use integral field spectroscopy from the PHANGS-MUSE survey, which resolves the ionised interstellar medium at ${\sim}50$ pc resolution in 19 nearby spiral galaxies, to study the origin of the diffuse ionised gas (DIG). We examine the…

We present a multiwavelength (ultraviolet, infrared, optical and CO) study of a set of luminous HII regions in M33: NGC 604, NGC 595, NGC 592, NGC 588 and IC131. We study the emission distribution in the interiors of the HII regions to…

星系天体物理 · 物理学 2011-02-11 Monica Relano , Robert C. Kennicutt

We present deep, narrowband imaging of the nearby spiral galaxy M101 and its satellites to analyze the oxygen abundances of their HII regions. Using CWRU's Burrell Schmidt telescope, we add to the narrowband dataset of the M101 Group,…

星系天体物理 · 物理学 2023-07-17 Ray Garner , J. Christopher Mihos , Paul Harding , Aaron E. Watkins , Stacy S. McGaugh

We present spectroscopic observations of diffuse ionized gas (DIG) in M33 near the HII region NGC 604. We present the first detection of [OI] 6300 in the DIG of M33, one of the critical lines for distinguishing photo- from shock ionization…

天体物理学 · 物理学 2009-11-11 E. S. Voges , R. A. M. Walterbos

We present deep, narrowband imaging of the nearby spiral galaxy M101 and its group environment to search for star-forming dwarf galaxies and outlying HII regions. Using the Burrell Schmidt telescope, we target the brightest emission lines…

星系天体物理 · 物理学 2021-07-14 Ray Garner , J. Christopher Mihos , Paul Harding , Aaron E. Watkins

A number of very small isolated HII regions have been discovered at projected distances up to 30 kpc from their nearest galaxy. These HII regions appear as tiny emission line objects in narrow band images obtained by the NOAO Survey for…

天体物理学 · 物理学 2015-06-24 E. V. Ryan-Weber , G. R. Meurer , K. C. Freeman , M. E. Putman , R. L. Webster , the SINGG team

We present a new catalog of HII regions in M31. The full disk of the galaxy is covered in a 2.2 deg^2 mosaic of 10 fields observed with the Mosaic Camera as part of the Local Group Galaxies survey. We used HIIphot, a code for automated…

宇宙学与河外天体物理 · 物理学 2015-05-30 Mohaddesseh Azimlu , Ryan Marciniak , Pauline Barmby

In this paper we make a quantitative study of the hypothesis that the diffuse H-alpha emitted from the discs of spiral galaxies owes its origin to the ionizing photons escaping from HII regions. We use the H-alpha measurements of the…

天体物理学 · 物理学 2009-11-07 A. Zurita , J. E. Beckman , M. Rozas , S. Ryder

We investigate the ionized gas kinematics of HII regions in the disk of NGC 7331 using integral field unit data collected with the Circumgalactic H$\alpha$ Spectrograph (CH$\alpha$S). NGC 7331 is a well-studied nearby galaxy with HII…

The Diffuse Ionized Gas (DIG) contributes to the nebular emission of galaxies, resulting in emission line flux ratios that can be significantly different from those produced by HII regions. Comparing the emission of [SII]6717,31 between…

星系天体物理 · 物理学 2021-09-29 F. Mannucci , F. Belfiore , M. Curti , G. Cresci , R. Maiolino , A. Marasco , A. Marconi , M. Mingozzi , G. Tozzi , A. Amiri

We present narrowband H-alpha imaging data of a small survey of nearby edge-on spiral galaxies, aiming at the detection of `extraplanar' diffuse ionized gas (DIG). A few of our studied edge-on spirals show signs of disk-halo interaction…

天体物理学 · 物理学 2007-05-23 J. Rossa , R. -J. Dettmar

We present results of KPNO 4-m optical spectroscopy of discrete emission-line nebulae and regions of diffuse ionized gas (DIG) in M31. Long-slit spectra of 16 positions in the NE half of M31 were obtained over a 5-15 kpc range in radial…

天体物理学 · 物理学 2009-10-31 V. C. Galarza , R. A. M. Walterbos , R. Braun

We show data from the Survey of Ionization in Neutral Gas Galaxies (SINGG) and Survey of Ultraviolet emission in Neutral Gas Galaxies (SUNGG) which survey the star formation properties of HI selected galaxies as traced by H-alpha and…

天体物理学 · 物理学 2009-11-13 Gerhardt R. Meurer , O. Ivy Wong , Daniel J. Hanish

We present a study of the diffuse ionized gas (DIG) in three Sculptor group galaxies: NGC 55, NGC 253, and NGC 300. The study is based on narrow band imagery in H-alpha+[NII](6548+6583A) and [SII] (6717+6731A). We find that DIG contributes…

天体物理学 · 物理学 2009-10-28 Charles G. Hoopes , Rene A. M. Walterbos , Bruce E. Greenawalt

In this work, we investigate the contribution of dust scattering to the diffuse H-alpha emission observed in nearby galaxies. As initial conditions for the spatial distribution of HII regions, gas, and dust, we take three Milky Way-like…

星系天体物理 · 物理学 2016-02-29 Y. Ascasibar , G. Guidi , J. Casado , C. Scannapieco , A. I. Díaz
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