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Printed by Marianne Doyle May 30, 05 9:26 HOPCAT2005TabSep.txt Page 1/192 1 2 3 4 5 6 7 8 9 10 11 12 13 14 15 16 17 18 19 20 21 22 23 24 25 26 27 28 29 30 31 32 33 ID_Numbers HicatName RA Dec Velocity Velocity Width Peak Flux Density Integrated Flux Optical Semi-Major Axis Optical Sem i-Minor Axis Optical Angle 6dF Velocity NED Velocity Match Class) Optical RA Degrees Optical Dec Degrees Optical RA H:M:S Opt ical Dec D:M:S Blue Magnitude Red Magnitude I Magnitude Blue SuperCOS Plate No. Red SuperCOS Plate No. I SuperCOS Plate No. l b Ext inction RA Position Sep Dec Position Sep Galaxy Position Sep AxisRatio Galaxy Name Morphology ID hipass_name ra dec vel_mom width_50max Sp Sint A_IMAGE B_IMAGE THETA_IMAGE Velocity_6dF Velocity_Ned Class(Match ed_choice) CorrectedSExRA CorrectedSExDec Matched_RA_H:M:S Matched_Dec_D:M:S Blue_Mag_AUTO_Calibrated Red_Mag_AUTO_Calabrated I_M ag_AUTO_Calibrated BluePlateNumber RedPlateNumber InfraSCosPlateNumber HicatExtl HicatExtb HicatExt DiffRaArcMin DiffDecArcM in GalSepArcMin AxisRatio Galaxy Name Morphology 1 HIPASSJ0146-89 01:56:13.1 -89:18:49 2452.8 228 0.068 12.3 33.156 13.498 21.4 XXXXX 2429 60 25.5098156 -89 .3343882 01:42:02.3 -89:20:03.7 13.7277 13.3693 14.3832 3665 17829 19408 302.7155 -27.7873 0.1347 2.5093 1.2466 2.8 013 2.4564 NGC 2573 SAB(rs+)c 2 HIPASSJ2311-89 23:08:01.3 -89:06:38 2525.4 160.5 0.2035 34 21.448 6.954 18.1 XXXXX 2558 40 346.8899988 -89 .1162463 23:07:33.5 -89:06:58.4 14.9107 14.5471 14.5864 3665 17829 19408 303.3709 -27.928 0.1459 0.1072 0.3414 0.3579 3.0 843 NGC 2573B IBm? pec 3 HIPASSJ0852-88 08:54:24.7 -88:03:59 4974.3 200.8 0.042 6.1 16.249 9.449 -51.7 XXXXX XXXXX 50 133.2599929 -88 .0899484 08:53:02.3 -88:05:23.8 14.99 14.6155 XXXXX 3665 17829 19408 301.0809 -26.1277 0.1391 0.69 1.4136 1.5 73 1.7197 ESO 001- G 005 Sa-b 4 HIPASSJ1427-87 14:30:16.5 -87:48:45 2251.4 312.7 0.118 27.4 48.614 12.453 -28 XXXXX 2245 60 216.8420763 -87 .7718849 14:27:22.0 -87:46:18.7 13.3267 13.1593 15.794 3665 17829 19408 303.9418 -25.1374 0.1265 1.6797 -2.4369 2.9 596 3.9038 ESO 001- G 006 SA:(rs)bc: 5 HIPASSJ1532-87 15:33:07.6 -87:26:11 2281.5 153 0.0814 11.3 44.92 9.087 -82.1 XXXXX 2357 60 232.8281486 -87 .4364342 15:31:18.7 -87:26:11.1 13.9525 13.6469 13.9095 2963 16259 16156 304.7682 -25.1647 0.1209 1.2171 0.0027 1.2 171 4.9433 ESO 008- G 008 Im 6 HIPASSJ1711-87 17:12:01.1 -87:23:35 2311.8 70 0.0604 4.3 14.588 10.616 24.6 XXXXX XXXXX 50 257.3211895 -87 .4122297 17:09:17.0 -87:24:44.0 15.1454 14.7451 15.5099 3505 17049 19240 305.564 -26.008 0.1732 1.8582 1.1504 2.1855 1.3742 ESO 009- G 005 SB(s)m: 7 HIPASSJ0504-87 05:02:47.8 -87:02:08 1758.5 60.9 0.1051 6.7 22.519 11.44 -26.8 XXXXX 1667 60 76.0980178 -87 .0302814 05:04:23.5 -87:01:49.0 15.3671 14.7112 16.9204 3859 16469 19310 299.932 -28.4495 0.1343 1.2387 -0.3164 1.2785 1.9 684 ESO 004- G 017 IB(s)m: 8 HIPASSJ0606-86 06:04:29.6 -86:35:50 1860.3 417 0.1261 31.6 60.904 12.883 -9.8 XXXXX 1809 60 91.4146295 -86 .631905 06:05:39.5 -86:37:54.8 12.9389 12.4881 12.1958 6791 16560 17437 299.1661 -27.7701 0.1401 1.0321 2.081 2.3229 4.7 275 ESO 005- G 004 Sb: sp 10 HIPASSJ1112-86 11:14:35.2 -86:20:15 2186.4 47.3 0.0523 2.7 9.193 6.467 13.6 XXXXX XXXXX 10 168.326603 -86 .3081702 11:13:18.3 -86:18:29.4 16.0418 15.5599 15.9495 4210 15450 17119 301.2914 -23.7785 0.2429 1.2316 -1.7598 2.1 48 1.4215 XXXXX XXXXX 12 HIPASSJ0519-86 05:14:45.6 -86:15:29 1844.1 128.6 0.0372 4.3 12.612 9.495 44 XXXXX XXXXX 50 79.0814731 -86 .2491177 05:16:19.5 -86:14:56.8 15.1461 14.5538 14.7222 3859 16469 19310 299.0431 -28.6066 0.1594 1.5347 -0.5363 1.6 257 1.3283 2MASX J05161938- XXXXX 13 HIPASSJ2037-86 20:41:03.1 -86:06:02 5102.2 97.6 0.055 6.2 10.899 9.203 64.5 XXXXX XXXXX 10 310.1993761 -86 .0683572 20:40:47.8 -86:04:06.0 15.4757 15.1599 15.0649 2562 16174 16304 306.8851 -28.8674 0.1519 0.2603 -1.9319 1.9 494 1.1843 2MASX J20404771- XXXXX 14 HIPASSJ1929-86 19:29:59.7 -86:00:52 2444.4 205.3 0.0826 11.5 47.915 20.597 21.6 XXXXX 2432 60 292.7494982 -86 .0148978 19:30:59.8 -86:00:53.6 13.4501 13.1906 13.1557 2477 15805 18457 307.3717 -27.7257 0.1332 1.0456 0.0272 1.0 46 2.3263 ESO 010- G 004 SB(rs)d 15 HIPASSJ0958-85 09:58:39.7 -85:45:54 1976.1 63.5 0.0272 2.1 XXXXX XXXXX XXXXX XXXXX XXXXX 20 XXXXX XXXXX XXX XX XXXXX XXXXX XXXXX XXXXX 3897 16981 15459 299.76 -24.0055 0.1805 XXXXX XXXXX XXXXX XXXXX XXXXX XXXXX 18 HIPASSJ0100-85 01:00:09.9 -85:32:15 4657.7 287.6 0.0454 10.4 30.651 5.84 -26 XXXXX 4640 60 15.1885805 -85 .5232392 01:00:45.2 -85:31:23.6 15.2965 14.9893 14.9692 2563 16683 19302 302.7327 -31.5874 0.1046 0.6889 -0.8556 1.0 985 5.2485 ESO 002- G 012 Sc 20 HIPASSJ1821-85 18:21:13.6 -85:21:48 2541.3 241.5 0.077 18.9 42.612 27.023 -78.5 XXXXX 2512 42 275.6468661 -85 .4059238 18:22:35.2 -85:24:21.3 12.3804 12.2662 11.8953 2477 15805 18457 308.0659 -26.4256 0.1707 1.6425 2.5554 3.0 377 1.5769 NGC 6438A S pec (Ring B) 21 HIPASSJ1740-85 17:38:08.7 -85:18:08 2437.4 270.8 0.0414 7.3 43.058 30.401 -88.1 XXXXX 2418 60 264.8835856 -85 .310346 17:39:32.0 -85:18:37.2 12.5594 12.3347 12.0744 3505 17049 19240 307.8761 -25.5652 0.1413 1.7053 0.4874 1.7736 1.4 163 ESO 009- G 010 SA(s)c 27 HIPASSJ1242-84 12:42:37.5 -84:28:12 2305.1 170 0.0646 9 23.419 18.317 -28.1 XXXXX 2303 60 190.514551 -84 .464348 12:42:03.4 -84:27:51.6 13.923 13.2416 13.353 4210 15450 17119 302.7036 -21.6022 0.1334 0.8197 -0.3391 0.8871 1.2 785 ESO 007- G 006 SA(s)d 29 HIPASSJ1941-84 19:41:38.7 -84:17:00 2516.9 136.5 0.0781 9.7 20.503 13.039 53 XXXXX 2578 60 295.0560447 -84 .2733081 19:40:13.4 -84:16:23.9 15.0014 14.6041 14.5482 2477 15805 18457 309.2676 -28.228 0.1629 2.1248 -0.6015 2.2083 1.5 724 ESO 010- G 006 SB(s)m 30 HIPASSJ0324-84 03:25:04.9 -84:07:49 4986.4 250.4 0.0345 6.6 25.637 12.487 6 XXXXX XXXXX 50 51.0152157 -84 Monday May 30, 2005 HOPCAT2005TabSep.txt 1/192 Printed by Marianne Doyle May 30, 05 9:26 HOPCAT2005TabSep.txt Page 2/192 .1600262 03:24:03.6 -84:09:36.0 14.3951 13.7678 13.6986 2565 16348 19301 298.6508 -31.6623 0.1289 1.562 1.7849 2.3 718 2.0531 ESO 003- G 015 SB(s)dm: 33 HIPASSJ0648-84 06:48:07.2 -84:05:47 5287.9 129.6 0.0284 3.5 XXXXX XXXXX XXXXX XXXXX XXXXX 20 XXXXX XXXXX XXX XX XXXXX XXXXX XXXXX XXXXX 6791 16560 17437 296.3003 -27.0579 0.208 XXXXX XXXXX XXXXX XXXXX XXXXX XXXXX 37 HIPASSJ0159-83 01:59:32.6 -83:59:33 3555.4 99.6 0.063 6.6 30.295 26.852 23.2 XXXXX 3413 60 30.0677205 -83 .9867967 02:00:16.2 -83:59:12.4 13.0686 12.4229 12.2762 2565 16348 19301 300.8412 -32.8569 0.1228 1.1427 -0.3422 1.1 928 1.1282 ESO 003- G 007 SAB(rs)c: pec 38 HIPASSJ0348-83 03:50:25.3 -83:58:56 5010.7 56.9 0.0962 5.1 22.243 17.161 -74.6 XXXXX XXXXX 50 57.3936902 -83 .9631663 03:49:34.4 -83:57:47.3 14.6207 13.9285 14.3088 3859 16469 19310 297.9762 -31.3147 0.1064 1.3339 -1.1434 1.7 569 1.2961 ESO 004- G 006 SA(s)m: 45 HIPASSJ1045-83 10:46:27.3 -83:50:36 2123.2 127.1 0.0488 5 9.733 2.55 65.6 XXXXX XXXXX 10 161.5755471 -83 .8451314 10:46:18.1 -83:50:42.4 17.1639 16.2741 16.6514 3897 16981 15459 299.4964 -21.8236 0.2351 0.2458 0.1079 0.2 684 3.8169 ESO 006- G 008 Sc 46 HIPASSJ0350-83 03:51:20.4 -83:50:27 1740.8 283 0.0985 27.2 51.868 30.046 -32.7 XXXXX 1735 60 58.0087316 -83 .8311893 03:52:02.0 -83:49:52.2 11.9005 11.5164 11.6411 3859 16469 19310 297.8351 -31.3927 0.114 1.1193 -0.5786 1.2 6 1.7263 IC 2051 SA(r)c 47 HIPASSJ0235-83 02:35:41.6 -83:50:13 3528.9 109.4 0.0354 2.9 12.462 8.096 -87.4 XXXXX XXXXX 10 38.35448 -83 .8625309 02:33:25.0 -83:51:45.1 16.0282 15.4558 14.931 2565 16348 19301 299.7211 -32.6278 0.1137 3.6567 1.5352 3.9 659 1.5393 ESO 003- G 011 Dwarf 52 HIPASSJ0427-83 04:27:35.3 -83:33:11 4835.6 241.7 0.0334 7.3 27.623 7.811 14 XXXXX 4835 60 66.8730306 -83 .5510448 04:27:29.5 -83:33:03.7 14.4367 13.9518 14.1639 3859 16469 19310 296.8594 -30.7828 0.1163 0.1621 -0.1206 0.2 02 3.5364 ESO 004- G 013 SB(s)c: pec 54 HIPASSJ0909-83 09:09:46.8 -83:29:24 2033.1 207.4 0.0247 3.9 XXXXX XXXXX XXXXX XXXXX XXXXX 20 XXXXX XXXXX XXX XX XXXXX XXXXX XXXXX XXXXX 3897 16981 15459 297.0983 -23.3138 0.1269 XXXXX XXXXX XXXXX XXXXX XXXXX XXXXX 57 HIPASSJ0138-83 01:38:46.5 -83:22:17 4894.3 338 0.0578 10.8 24.967 11.546 21.1 XXXXX 4907 60 24.7015783 -83 .3645421 01:38:48.3 -83:21:52.3 14.3982 13.7364 13.6467 2565 16348 19301 301.3031 -33.6065 0.1444 0.0542 -0.4108 0.4 144 2.1624 ESO 003- G 003 SAB(rs)c 58 HIPASSJ0551-83 05:52:04.0 -83:19:00 4802.3 223.1 0.0405 7.5 12.395 7.451 -55.9 XXXXX XXXXX 50 87.994698 -83 .2973814 05:51:58.7 -83:17:50.5 15.4096 14.7356 14.8096 3859 16469 19310 295.5669 -28.6474 0.1491 0.1536 -1.1571 1.1 673 1.6635 ESO 004- G 023 SBc: pec 62 HIPASSJ1104-83 11:04:04.6 -83:15:41 2065.1 129.4 0.0378 3.7 13.055 1.978 -21.5 XXXXX XXXXX 50 166.2575238 -83 .249676 11:05:01.8 -83:14:58.8 17.0816 16.3158 16.4871 4210 15450 17119 299.677 -21.0789 0.2717 1.6796 -0.7028 1.8207 6.6001 ESO 007- G 003 Sc 66 HIPASSJ1357-83 13:57:57.6 -83:03:33 2445.1 137.1 0.1667 18.8 44.486 39.912 10.3 XXXXX XXXXX 50 209.4568012 -83 .0800622 13:57:49.6 -83:04:48.2 13.1394 12.6269 12.6771 2963 16259 16156 305.0475 -20.4623 0.1779 0.2404 1.2537 1.2 766 1.1146 ESO 008- G 004 SAB(rs)cd 67 HIPASSJ1741-82 17:40:46.4 -82:56:54 5157.1 122.3 0.0431 4.9 15.072 13.455 -62.2 XXXXX XXXXX 50 265.3901708 -83 .0064593 17:41:33.6 -83:00:23.2 14.4986 14.0572 13.8772 3505 17049 19240 310.3353 -24.7953 0.1419 1.4439 3.4876 3.7 746 1.1202 ESO 009- G 011 Sa-b 70 HIPASSJ1600-82 16:00:41.5 -82:55:22 2566 207.7 0.0332 5.3 30.925 14.216 -20.5 XXXXX XXXXX 50 239.910563 -82 .9140792 15:59:38.5 -82:54:50.6 14.0519 13.3339 13.2306 3505 17049 19240 308.5462 -22.2202 0.1418 1.9406 -0.5219 2.0 096 2.1754 ESO 009- G 001 SAB(s)b: 74 HIPASSJ2141-82 21:41:22.6
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  • Outflows in the Seyfert 2 Galaxy NGC 5643 Traced By

    Outflows in the Seyfert 2 Galaxy NGC 5643 Traced By

    Publications of the Astronomical Society of Australia (2018), 35, e040, 8 pages doi:10.1017/pasa.2018.31 Research Paper Outflows in the Seyfert 2 galaxy NGC 5643 traced by the [S III] emission Rogemar A. Riffel1,C.Hekatelyne1 and Izabel C. Freitas1,2 1Departamento de Física, CCNE, Universidade Federal de Santa Maria, Santa Maria, 97105-900 RS, Brazil and 2Colégio Politécnico, Universidade Federal de Santa Maria, Santa Maria, 97105-900 RS, Brazil Abstract We use Gemini Multi-Object Spectrograph Integral Field Unit observations of the inner 285 × 400 pc2 region of the Seyfert 2 galaxy NGC 5643 to map the [S III]λ9069 emission line flux distribution and kinematics, as well as the stellar kinematics, derived by fitting the Ca IIλλλ8498,8542,8662 triplet, at a spatial resolution of 45 pc. The stellar velocity field shows regular rotation, with a projected velocity of − ◦ − 100 km s 1 and kinematic major axis along a position angle of –36 . A ring of low stellar velocity dispersion values (∼70 km s 1), attributed to young/intermediate age stellar populations, is seen surrounding the nucleus with a radius of 50 pc. We found that the [S III] flux distribu- tion shows an elongated structure along the east–west direction and its kinematics is dominated by outflows within a bi-cone at an ionised − gas outflow rate of 0.3 M yr 1. In addition, velocity slices across the [S III]λ9069 emission line reveal a kinematic component attributed to rotation of gas in the plane of the galaxy. Keywords: galaxies: active – galaxies: individual (NGC 5643) – galaxies: kinematics – galaxies: Seyfert (Received April 10, 2018; revised 7 July 2018; accepted August 16, 2018) 1.
  • Neutral Hydrogen in Nearby Dwarf Galaxies B¨Arbel S

    Neutral Hydrogen in Nearby Dwarf Galaxies B¨Arbel S

    Dwarf Galaxies: From the Deep Universe to the Present Proceedings IAU Symposium No. 344, 2018 c 2018 International Astronomical Union K. McQuinn & S. Stierwalt, eds. DOI: 00.0000/X000000000000000X Neutral Hydrogen in Nearby Dwarf Galaxies B¨arbel S. Koribalski CSIRO Astronomy and Space Science, Australia Telescope National Facility PO Box 76, Epping, NSW 1710, Australia email: [email protected] Abstract. Here I briefly highlight our studies of the gas content, kinematics and star formation in nearby dwarf galaxies (D < 10 Mpc) based on the `Local Volume H i Survey' (LVHIS, Koribalski et al. 2018), which was conducted with the Australia Telescope Compact Array (ATCA). The LVHIS sample consists of nearly 100 galaxies, including new discoveries, spanning a large diversity in size, shape, mass and degree of peculiarity. The hydrogen properties of dwarf galaxies in two nearby groups, Sculptor and CenA / M83, are analysed and compared with many rather isolated dwarf galaxies. Around 10% of LVHIS galaxies are transitional or mixed-type dwarf galaxies (dIrr/dSph), the formation of which is explored. | I also provide a brief update on WALLABY Early Science, where we focus on studying the H i properties of galaxies as a function of environment. WALLABY (Dec < +30 degr, z < 0:26) is conducted with the Australian SKA Pathfinder (ASKAP), a ∼6-km diameter array of 36 × 12-m dishes, each equipped with wide-field (30 sq degr) Chequerboard Phased Array Feeds. Keywords. galaxies: kinematics and dynamics | galaxies: structure | radio lines: galaxies | surveys 1. LVHIS { The Local Volume H i Survey The LVHIS project provides high-resolution H i spectral line and 20-cm radio contin- uum data products for nearly 100 nearby galaxies, based on over 2500 hours of ATCA observations.
  • Exploding Star in NGC 2397 31 March 2008

    Exploding Star in NGC 2397 31 March 2008

    Exploding star in NGC 2397 31 March 2008 Camera for Surveys (ACS). One atypical feature of this Hubble image is the view of supernova SN 2006bc taken when it was still fairly faint and its brightness on the increase. Astronomers from Queen's University Belfast in Northern Ireland, led by Professor of Astronomy Stephen J. Smartt, requested the image as part of a long project studying the massive exploding stars — supernovae. Exactly which types of star will explode and the lowest mass of star that can produce a supernova are not known. When a supernova is discovered in a nearby galaxy the group begins a painstaking search of earlier Hubble images of the same galaxy to locate the NGC 2397, pictured in this image from Hubble, is a star that later exploded; often one of hundreds of classic spiral galaxy with long prominent dust lanes millions of stars in the galaxy. This is a little like along the edges of its arms, seen as dark patches and sifting through days of CCTV footage to find one streaks silhouetted against the starlight. Hubble's frame showing a suspect. If the astronomers find a exquisite resolution allows the study of individual stars in star at the location of the later explosion, they may nearby galaxies. Located nearly 60 million light-years work out the mass and type of star from its away from Earth, the galaxy NGC 2397 is typical of most spirals, with mostly older, yellow and red stars in its brightness and colour. Only six such stars have central portion, while star formation continues in the been identified before they exploded and the outer, bluer spiral arms.
  • Dust and CO Emission Towards the Centers of Normal Galaxies, Starburst Galaxies and Active Galactic Nuclei�,�� I

    Dust and CO Emission Towards the Centers of Normal Galaxies, Starburst Galaxies and Active Galactic Nuclei, I

    A&A 462, 575–579 (2007) Astronomy DOI: 10.1051/0004-6361:20047017 & c ESO 2007 Astrophysics Dust and CO emission towards the centers of normal galaxies, starburst galaxies and active galactic nuclei, I. New data and updated catalogue M. Albrecht1,E.Krügel2, and R. Chini3 1 Instituto de Astronomía, Universidad Católica del Norte, Avenida Angamos 0610, Antofagasta, Chile e-mail: [email protected] 2 Max-Planck-Institut für Radioastronomie (MPIfR), Auf dem Hügel 69, 53121 Bonn, Germany 3 Astronomisches Institut der Ruhr-Universität Bochum (AIRUB), Universitätsstr. 150 NA7, 44780 Bochum, Germany Received 6 January 2004 / Accepted 27 October 2006 ABSTRACT Aims. The amount of interstellar matter in a galaxy determines its evolution, star formation rate and the activity phenomena in the nucleus. We therefore aimed at obtaining a data base of the 12CO line and thermal dust emission within equal beamsizes for galaxies in a variety of activity stages. Methods. We have conducted a search for the 12CO (1–0) and (2–1) transitions and the continuum emission at 1300 µmtowardsthe centers of 88 galaxies using the IRAM 30 m telescope (MRT) and the Swedish ESO Submillimeter Telescope (SEST). The galaxies > are selected to be bright in the far infrared (S 100 µm ∼ 9 Jy) and optically fairly compact (D25 ≤ 180 ). We have applied optical spectroscopy and IRAS colours to group the galaxies of the entire sample according to their stage of activity into three sub-samples: normal, starburst and active galactic nuclei (AGN). The continuum emission has been corrected for line contamination and synchrotron contribution to retrieve the thermal dust emission.
  • Atlas Menor Was Objects to Slowly Change Over Time

    Atlas Menor Was Objects to Slowly Change Over Time

    C h a r t Atlas Charts s O b by j Objects e c t Constellation s Objects by Number 64 Objects by Type 71 Objects by Name 76 Messier Objects 78 Caldwell Objects 81 Orion & Stars by Name 84 Lepus, circa , Brightest Stars 86 1720 , Closest Stars 87 Mythology 88 Bimonthly Sky Charts 92 Meteor Showers 105 Sun, Moon and Planets 106 Observing Considerations 113 Expanded Glossary 115 Th e 88 Constellations, plus 126 Chart Reference BACK PAGE Introduction he night sky was charted by western civilization a few thou - N 1,370 deep sky objects and 360 double stars (two stars—one sands years ago to bring order to the random splatter of stars, often orbits the other) plotted with observing information for T and in the hopes, as a piece of the puzzle, to help “understand” every object. the forces of nature. The stars and their constellations were imbued with N Inclusion of many “famous” celestial objects, even though the beliefs of those times, which have become mythology. they are beyond the reach of a 6 to 8-inch diameter telescope. The oldest known celestial atlas is in the book, Almagest , by N Expanded glossary to define and/or explain terms and Claudius Ptolemy, a Greco-Egyptian with Roman citizenship who lived concepts. in Alexandria from 90 to 160 AD. The Almagest is the earliest surviving astronomical treatise—a 600-page tome. The star charts are in tabular N Black stars on a white background, a preferred format for star form, by constellation, and the locations of the stars are described by charts.