Zobrazeno 1 - 10
of 165
pro vyhledávání: '"Hodge, Paul W."'
Autor:
Hwang, Narae, Park, Hong Soo, Lee, Myung Gyoon, Lim, Sungsoon, Hodge, Paul W., Kim, Sang Chul, Miller, Bryan, Weisz, Daniel
Publikováno v:
2014 ApJ 783 49
We present a spectroscopic study of the four extended star clusters (ESCs) in NGC 6822 based on the data obtained with Gemini Multi-Object Spectrograph (GMOS) on the Gemini-South 8.1m telescope. Their radial velocities derived from the spectra range
Externí odkaz:
http://arxiv.org/abs/1401.2492
Autor:
Johnson, L. Clifton, Seth, Anil C., Dalcanton, Julianne J., Caldwell, Nelson, Fouesneau, Morgan, Gouliermis, Dimitrios A., Hodge, Paul W., Larsen, Soeren S., Olsen, Knut A. G., Roman, Izaskun San, Sarajedini, Ata, Weisz, Daniel R., Williams, Benjamin F., Beerman, Lori C., Bianchi, Luciana, Dolphin, Andrew E., Girardi, Leo, Guhathakurta, Puragra, Kalirai, Jason, Lang, Dustin, Monachesi, Antonela, Nanda, Sanjay, Rix, Hans-Walter, Skillman, Evan D.
Publikováno v:
Astrophysical Journal, 752, 95 (2012)
The Panchromatic Hubble Andromeda Treasury (PHAT) survey is an on-going Hubble Space Telescope (HST) multi-cycle program to obtain high spatial resolution imaging of one-third of the M31 disk at ultraviolet through near-infrared wavelengths. In this
Externí odkaz:
http://arxiv.org/abs/1204.3091
Autor:
Johnson, L. Clifton, Seth, Anil C., Dalcanton, Julianne J., Caldwell, Nelson, Gouliermis, Dimitrios A., Hodge, Paul W., Larsen, Soeren S., Olsen, Knut A. G., Roman, Izaskun San, Sarajedini, Ata, Weisz, Daniel R., Collaboration, the PHAT
The Panchromatic Hubble Andromeda Treasury (PHAT) is an on-going Hubble Space Telescope (HST) multi-cycle program that will image one-third of the M31 disk at high resolution, with wavelength coverage from the ultraviolet through the near-infrared. T
Externí odkaz:
http://arxiv.org/abs/1107.2668
Autor:
Krienke, O. K., Hodge, Paul W.
This paper reports on a survey of star clusters in M31 based on archival images from the Hubble Space Telescope. Paper I (Krienke and Hodge 2007) reported results from images obtained with the Wide Field/Planetary Camera 2 (WFPC2) and this paper repo
Externí odkaz:
http://arxiv.org/abs/0711.4563
Autor:
Massey, Philip, McNill, Reagin T., Olsen, K. A. G., Hodge, Paul W., Blaha, Cynthia, Jacoby, George H., Smith, R. C., Strong, Shay B.
We describe a search for H-alpha emission-lined stars in M31, M33, and seven dwarfs in or near the Local Group (IC 10, NGC 6822, WLM, Sextans B, Sextans A, Pegasus and the Phoenix dwarf) using interference filter imaging with the KPNO and CTIO 4-m te
Externí odkaz:
http://arxiv.org/abs/0709.1267
Autor:
Massey, Philip, Olsen, K. A. G., Hodge, Paul W., Jacoby, George H., McNeill, Reagin T., Smith, R. C, Strong, Shay B.
Publikováno v:
Astron.J.133:2393-2417,2007
We have obtained UBVRI images with the Kitt Peak and Cerro Tololo 4-m telescopes and Mosaic cameras of seven dwarfs in (or near) the Local Group, all of which have known evidence of recent star formation: IC10, NGC 6822, WLM, Sextans B, Sextans A, Pe
Externí odkaz:
http://arxiv.org/abs/astro-ph/0702236
Publikováno v:
Astron.J.132:2539-2555,2006
We find 9 nuclear cluster candidates in a sample of 14 edge-on, late-type galaxies observed with HST/ACS. These clusters have magnitudes (M_I ~ -11) and sizes (r_eff ~ 3pc) similar to those found in previous studies of face-on, late-type spirals and
Externí odkaz:
http://arxiv.org/abs/astro-ph/0609302
From observations of edge-on, late-type galaxies, we present morphological evidence that some nuclear star clusters have experienced in situ star formation. We find three nuclear clusters that, viewed from the edge-on perspective, have both a compact
Externí odkaz:
http://arxiv.org/abs/astro-ph/0606066
Autor:
Massey, Philip, Olsen, K. A. G., Hodge, Paul W., Strong, Shay B., Jacoby, George H., Schlingman, Wayne, Smith, R. C.
Publikováno v:
Astron.J.131:2478-2486,2006
We present UBVRI photometry obtained from Mosaic images of M31 and M33 using the KPNO 4-m telescope. The survey covers 2.2 sq degrees of M31, and 0.8 sq degrees of M33, chosen so as to include all of the regions currently active in forming massive st
Externí odkaz:
http://arxiv.org/abs/astro-ph/0602128