Tartalom
Képek
Kép feltöltése
DSS Images Other Images
Kapcsolódó cikkek
The ISOPHOT 170 μm Serendipity Survey II. The catalog of optically identified galaxies%
The ISOPHOT Serendipity Sky Survey strip-scanning measurements covering≈15% of the far-infrared (FIR) sky at 170 μm were searched forcompact sources associated with optically identified galaxies. CompactSerendipity Survey sources with a high signal-to-noise ratio in at leasttwo ISOPHOT C200 detector pixels were selected that have a positionalassociation with a galaxy identification in the NED and/or Simbaddatabases and a galaxy counterpart visible on the Digitized Sky Surveyplates. A catalog with 170 μm fluxes for more than 1900 galaxies hasbeen established, 200 of which were measured several times. The faintest170 μm fluxes reach values just below 0.5 Jy, while the brightest,already somewhat extended galaxies have fluxes up to ≈600 Jy. For thevast majority of listed galaxies, the 170 μm fluxes were measured forthe first time. While most of the galaxies are spirals, about 70 of thesources are classified as ellipticals or lenticulars. This is the onlycurrently available large-scale galaxy catalog containing a sufficientnumber of sources with 170 μm fluxes to allow further statisticalstudies of various FIR properties.Based on observations with ISO, an ESA project with instruments fundedby ESA Member States (especially the PI countries: France, Germany, TheNetherlands and the UK) and with the participation of ISAS and NASA.Members of the Consortium on the ISOPHOT Serendipity Survey (CISS) areMPIA Heidelberg, ESA ISO SOC Villafranca, AIP Potsdam, IPAC Pasadena,Imperial College London.Full Table 4 and Table 6 are only available in electronic form at theCDS via anonymous ftp to cdsarc.u-strasbg.fr (130.79.128.5) or viahttp://cdsweb.u-strasbg.fr/cgi-bin/qcat?J/A+A/422/39
| Total magnitude, radius, colour indices, colour gradients and photometric type of galaxies
We present a catalogue of aperture photometry of galaxies, in UBVRI,assembled from three different origins: (i) an update of the catalogueof Buta et al. (1995) (ii) published photometric profiles and (iii)aperture photometry performed on CCD images. We explored different setsof growth curves to fit these data: (i) The Sersic law, (ii) The net ofgrowth curves used for the preparation of the RC3 and (iii) A linearinterpolation between the de Vaucouleurs (r(1/4) ) and exponential laws.Finally we adopted the latter solution. Fitting these growth curves, wederive (1) the total magnitude, (2) the effective radius, (3) the colourindices and (4) gradients and (5) the photometric type of 5169 galaxies.The photometric type is defined to statistically match the revisedmorphologic type and parametrizes the shape of the growth curve. It iscoded from -9, for very concentrated galaxies, to +10, for diffusegalaxies. Based in part on observations collected at the Haute-ProvenceObservatory.
| The H I-Rich Elliptical Galaxy NGC 5266
We present new ion{H}{1} images of the dust-lane elliptical galaxy NGC5266 already known from single-dish observations to contain a largeamount of ion{H}{1}. Our new data confirm that NGC 5266 contains ~2.4 x10(10) msun (for Hdeg = 50 kmsMp) of neutral hydrogen, i.e.more than most spiral galaxies of similar luminosity. The gas extends to~8(') each side of the nucleus, or 8 times the optical half-light radiusR_e. Surprisingly, most of the ion{H}{1} extends almost orthogonal tothe optical dust lane. A small fraction of the ion{H}{1} is associatedwith the dust lane and there are some hints of a faint warp connectingthe two structures. The ion{H}{1} distribution is somewhat clumpy andasymmetric, but the overall velocity field in the inner 4(') can besuccessfully modeled by assuming that the gas lies mainly in twoperpendicular planes - in the plane of the dust lane in the centralparts and orthogonal to this in the outer regions. Beyond the 4(')radius, the gas has a different structure and may be in two tidal tails,or an edge-on ring. Measurement of the ion{H}{1} rotation curve isaffected by asymmetries in the gas distribution, but the rotationvelocity is at least 250 kms at a radius of 4(') , and a flat rotationcurve of ~270 kms is consistent with the data. This would imply a valueof M / L_B ~8 at ~4 R_e. If the outermost ion{H}{1} is in an edge-onring, we estimate M / L_B ~16 at ~8 R_e. Comparing this with the valuederived from optical observations for the inner region we find anincrease of M / L_B by a factor ~2.7 at r ~4 R_e, and by 5.3 at r ~8R_e. The large amount of neutral gas observed in NGC 5266 (M_HI/L_B~0.2) and the ion{H}{1} morphology, suggest that this object may haveformed from the merger of two spiral galaxies. If so, NGC 5266 probablyrepresents a relatively old merger remnant since most of the ion{H}{1}gas appears settled.
| Redshift Distribution of Galaxies in the Southern Milky Way Region 210 degrees < L < 360 degrees and B < 15 degrees
Abstract image available at:http://adsabs.harvard.edu/cgi-bin/nph-bib_query?1996ApJS..107..521V&db_key=AST
| First data from the ISOPHOT FIR Serendipity survey.
The ISOPHOT Serendipity Survey fills the otherwise unused slew timebetween ISO's fine pointings with measurements in an unexploredwavelength regime near 200μm. First results of the Serendipity Surveydemonstrate its capabilities in the detection of extragalactic pointsources as well as in investigations of the galactic infrared cirrus.With the detection limit for point sources of ~1Jy more than 3000galaxies will be observed.
| The Catalog of Southern Ringed Galaxies
The Catalog of Southern Ringed Galaxies (CSRG) is a comprehensivecompilation of diameters, axis ratios, relative bar position angles, andmorphologies of inner and outer rings, pseudorings, and lenses in 3692galaxies south of declination -17 deg. The purpose of the catalog is toevaluate the idea that these ring phenomena are related to orbitalresonances with a bar or oval in galaxy potentials. The catalog is basedon visual inspection of most of the 606 fields of the Science ResearchCouncil (SRC) IIIa-J southern sky survey, with the ESO-B, ESO-R, andPalomar Sky surveys used as auxiliaries when needed for overexposed coreregions. The catalog is most complete for SRC fields 1-303 (mostly southof declination -42 deg). In addition to ringed galaxies, a list of 859mostly nonringed galaxies intended for comparison with other catalogs isprovided. Other findings from the CSRG that are not based on statisticsare the identification of intrinsic bar/ring misalignment; bars whichunderfill inner rings; dimpling of R'1pseudorings; pointy, rectangular, or hexagonal inner or outer ringshapes; a peculiar polar-ring-related system; and other extreme examplesof spiral structure and ring morphology.
| A search for IRAS galaxies behind the southern Milky Way
We systematically searched for IRAS galaxies with 60 micrometer fluxdensity larger than 0.6 Jy by using the UK Schmidt Infrared and IIIa-JAtlases in the Milky Way region (absolute value of b less than 15 deg)between l = 210 deg and 360 deg. We first selected about 4000 IRAS pointsources by using our far-infrared criteria, which are optimized for thesearch of IRAS galaxies behind the Milky Way region, and then inspectedvisually the optical counterparts of them on the Schmidt Atlas filmcopies. We found 966 IRAS sources associated with galaxy-like objects.The list of the objects is presented here with the IRAS source name,Galactic coordinates, IRAS flux densities, field number and emulsion ofthe Atlas, type and size of galaxy (-like) image, redshift,multiplicity, and cross-identification. Of these, 423 galaxies arealready cataloged in the Catalog of Galaxies and Quasars Observed in theIRAS Survey, and most of the remaining 543 galaxy candidates are newlyidentified in this search. Although the radial velocities are known foronly 387 galaxies, of which 60 were newly measured by us so far, weinferred the contamination by Galactic objects to be small from the goodcorrelation between the sky distributions of the newly identified galaxycandidates and the previously cataloged galaxies. In the regions wherethe Galactic molecular clouds dominate, almost all the sources were notidentified as galaxies. The detected galaxies are clustered in the threeregions around l = 240 deg, 280 deg, and 315 deg, where the projectednumber densities are higher than the whole-sky average of IRAS galaxiesof the same flux limit.
| General study of group membership. II - Determination of nearby groups
We present a whole sky catalog of nearby groups of galaxies taken fromthe Lyon-Meudon Extragalactic Database. From the 78,000 objects in thedatabase, we extracted a sample of 6392 galaxies, complete up to thelimiting apparent magnitude B0 = 14.0. Moreover, in order to considersolely the galaxies of the local universe, all the selected galaxieshave a known recession velocity smaller than 5500 km/s. Two methods wereused in group construction: a Huchra-Geller (1982) derived percolationmethod and a Tully (1980) derived hierarchical method. Each method gaveus one catalog. These were then compared and synthesized to obtain asingle catalog containing the most reliable groups. There are 485 groupsof a least three members in the final catalog.
| Photometry of luminous spiral galaxies in the direction of the Great Attractor
This paper presents photoelectric multiaperture BVI magnitudes for ahomogeneous sample of luminous spirals in the direction of the GreatAttractor. The total magnitudes B(T) and the mean colors (B - V) and (B- I) were determined for each galaxy and analyzed. The (B - I) colorchanges linearly with csc b over the range 3-10 and has a slope of 0.071mag. The A super bB values calculated from B - I agrees wellwith the A super bB values derived following the precepts ofBurstein and Heiles (1978). The (B - I) super b values show a slope of0.47 with log R. The corrected absolute magnitudes M superb,i,zB of spirals show little variation with luminosityclasses I, I-II, and II and have a dispersion of 0.85 mag. The samplewith well determined luminosities exhibits a uniform distribution overlog v up to v about 10,000 km/s. There is an indication that aselection-bias favoring higher luminosity galaxies sets in for spiralgalaxies with v greater than 10,000 km/s. The spirals with v less than10,000 km/s place a limit of about 500 km/s on peculiar velocities in ornear the Great Attractor.
| Redshifts of luminous spiral galaxies in the direction of the Great Attractor
The spatial distribution of a homogeneous samples of luminous spirals inthe direction of the 'Great Attractor' is studied. New radial velocitiesand published data yield redshifts for 94 percent of the sample. Thepresent survey, which does not include the cores of the Hydra andCentaurus clusters, shows no evidence for a major excess of velocitiesat or near the redshift of the Great Attractor. Luminous spirals withredshifts in the range 2000-4000 km/s are mainly distributed in a smallnumber of groups or clumps, whereas the spirals with redshifts in therange 4000-7000 km/s mostly appear to exhibit a rather smooth spatialdistribution.
| The supergalactic plane redshift survey
Redshift measurements, about 1000 of which are new, are presented for1314 galaxies in a survey toward the apex of the large-scale streamingflow for ellipticals. The velocity histogram shows that the excess ingalaxy number counts in this area is due to a substantial concentrationof galaxies with discrete peaks at V about 3000 km/s and V about 4500km/s. After correction for the sampling function, the centroid of thedensity distribution is found to be near V about 4500 km/s.Normalization to the more extensive SSRS survey, which was selected bythe same criteria, shows that the region studied contains a considerableoverdensity of galaxies from 2000 to 6000 km/s. This result is in goodagreement with the 'great attractor' model suggested by Lynden-Bell etal. (1988) which attributes the peculiar motions of elliptical galaxiesover a large region of space to an extensive mass overdensity whichincludes the Hydra-Centaurus and Pavo-Indus superclusters. The centroidof the density enhancement is also consistent with new data by Dresslerand Faber (1990) of peculiar motions of elliptical and spiral galaxies,both of which show a zero crossing of the Hubble line at approximately4500-5000 km/s.
| IRAS Faint Source Catalogue, version 2.0.
Not Available
| A survey of high-luminosity spirals in the direction of the great attractor
Luminosity-classification techniques have been used to study galaxies in33 SRC Schmidt fields centered on the position of 'The Great Attractor'.A catalog and finding charts are given for 191 spiral galaxies, whichare probably of DDO luminosity classes I, I-II, or II. Radial velocitiesof these objects should provide considerable insight into thethree-dimensional structure of this region of space. The surfacedistribution of galaxies in the survey area is seen to be stronglyaffected by Galactic absorption. It is therefore not clear if anysignificance should be attached to the observation that there is noobvious concentration of galaxies at, or near, the position of The GreatAttractor.
| A wide angle redshift survey of the Hydra-Centaurus region
Spectroscopic observations of 266 galaxies in the Hya-Cen region arereported. Redshift data obtained at 350-700 nm with dispersion 21 nm/mmusing the UNIT spectrograph and RPCS detector on the 1.9-m RadcliffeReflector telescope at SAO during March 1985, May 1986, and March 1987are presented in tables and graphs and briefly characterized. It isshown that the Hya supercluster is separated from the Cen superclusterby a large void at right ascension 11 h 40 min, declination -35 deg, andradial velocity 5200 km/sec; a bridge of galaxies at velocity about 3200km/sec connects the two superclusters.
| Dust and gas - Overview
Progress made in the study of dust and gas in elliptical galaxies overthe last 50 years is reviewed. The detection and measurement of dust,cool gas, warm gas, hot gas, and chemical abundances in ellipticals arediscussed. The spatial distribution of the dust and gas and the gaskinematics and dynamics are addressed. The status of knowledgeconcerning the sources and sinks of gas and the net balance of gas andconcerning the main heating and cooling mechanisms in ellipticalgalaxies is considered.
| Southern Galaxy Catalogue.
Not Available
| An optical and H I study of late-type low surface brightness galaxies
Neutral hydrogen and optical parameters are presented for 151 galaxiesof low surface brightness selected from UK Schmidt plates. The 21-cm H Iline was detected in 100 of these systems. It is found that the galaxiesshow the same trends of global properties with type as samples of brightgalaxies, while the data are consistent with the low surface brightness(LSB) galaxies being of systematically lower mass than bright galaxiesof the same type and linear dimensions. A constant value of hydrogenmass/(linear dimension)/squared is strongly suggested for LSB and brightgalaxies.
| UBV photometry of 262 southern galaxies
Multiaperture photometry of 262 bright southern galaxies in the JohnsonUBV system is given. Most of these are south of -30 deg declination,although some northward to -10 deg are included. A total of 169 objectshave published radial-velocity determinations. These provide distancesand enable construction of color-magnitude diagrams for this subset ofobjects through a physical diameter of 2.0 kpc (with H = 100). Thetwo-color diagrams for the inner regions of the galaxies differ fromthose of integrated galaxies due to the color changes towards theircenters. Comparison with theoretical models of Larson and Tinsley (1978)suggest that the colors of the inner portions of most ellipticals andlenticulars are consistent with their having all stars formed at nearlyone epoch with little subsequent star formation, while for spiralslarger amounts of star formation, either in bursts or continuously, aresuggested. This simple picture is complicated by the presence of certainobjects having peculiar colors indicative of large amounts of recentstar formation.
|
Új cikk hozzáadása
Kapcsolódó hivatkozások
- - (nincs kapcsolódó hivatkozás) -
Új link hozzáadása
Besorolás csoportokba:
|
Pozíciós és asztrometriai adatok
Katalógusok és elnevezések:
|
