Chandra Observations of Arp 220

S. Shaked; J. C. McDowell; D.~L. Clements; K. Borne; S. Lamb; A. C. Baker; Carole Mundell; Luis Colina

Chandra Observations of Arp 220

S. Shaked, J. C. McDowell, D.~L. Clements, K. Borne, S. Lamb, A. C. Baker, Carole Mundell, Luis Colina

Department of Physics

Research output: Contribution to journal › Article › peer-review

Abstract

We analyze recent Chandra data of the ultraluminous infrared galaxy Arp 220 and compare it to previously acquired ROSAT data. Chandra's high resolution allows us to see that a concentrated source of hard X-ray emission is located within 2'' (<1 kpc) of the radio/infrared nuclei. By comparing our Chandra data to Hα data, we find that the extended X-ray nebula coincides with the Hα morphology thus supporting the double-bubble ``superwind'' theory of Heckman et al. 1996. Finally, we find that the southern cluster seen in the ROSAT image is resolved into point-like sources, the positions of which coincide with bright optical galaxies. Funding was provided by the NSF REU program.

Original language	English
Pages (from-to)	1460
Journal	Bulletin of the American Astronomical Society
Volume	32
Publication status	Published - Dec 2000

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@article{9c2849995f9d46fb94b5e40325e49da2,

title = "Chandra Observations of Arp 220",

abstract = "We analyze recent Chandra data of the ultraluminous infrared galaxy Arp 220 and compare it to previously acquired ROSAT data. Chandra's high resolution allows us to see that a concentrated source of hard X-ray emission is located within 2'' (<1 kpc) of the radio/infrared nuclei. By comparing our Chandra data to Hα data, we find that the extended X-ray nebula coincides with the Hα morphology thus supporting the double-bubble ``superwind'' theory of Heckman et al. 1996. Finally, we find that the southern cluster seen in the ROSAT image is resolved into point-like sources, the positions of which coincide with bright optical galaxies. Funding was provided by the NSF REU program. ",

author = "S. Shaked and McDowell, {J. C.} and D.~L. Clements and K. Borne and S. Lamb and Baker, {A. C.} and Carole Mundell and Luis Colina",

year = "2000",

month = dec,

language = "English",

volume = "32",

pages = "1460",

journal = "Bulletin of the American Astronomical Society",

issn = "0002-7537",

publisher = "American Astronomical Society",

}

TY - JOUR

T1 - Chandra Observations of Arp 220

AU - Shaked, S.

AU - McDowell, J. C.

AU - Clements, D.~L.

AU - Borne, K.

AU - Lamb, S.

AU - Baker, A. C.

AU - Mundell, Carole

AU - Colina, Luis

PY - 2000/12

Y1 - 2000/12

N2 - We analyze recent Chandra data of the ultraluminous infrared galaxy Arp 220 and compare it to previously acquired ROSAT data. Chandra's high resolution allows us to see that a concentrated source of hard X-ray emission is located within 2'' (<1 kpc) of the radio/infrared nuclei. By comparing our Chandra data to Hα data, we find that the extended X-ray nebula coincides with the Hα morphology thus supporting the double-bubble ``superwind'' theory of Heckman et al. 1996. Finally, we find that the southern cluster seen in the ROSAT image is resolved into point-like sources, the positions of which coincide with bright optical galaxies. Funding was provided by the NSF REU program.

AB - We analyze recent Chandra data of the ultraluminous infrared galaxy Arp 220 and compare it to previously acquired ROSAT data. Chandra's high resolution allows us to see that a concentrated source of hard X-ray emission is located within 2'' (<1 kpc) of the radio/infrared nuclei. By comparing our Chandra data to Hα data, we find that the extended X-ray nebula coincides with the Hα morphology thus supporting the double-bubble ``superwind'' theory of Heckman et al. 1996. Finally, we find that the southern cluster seen in the ROSAT image is resolved into point-like sources, the positions of which coincide with bright optical galaxies. Funding was provided by the NSF REU program.

M3 - Article

SN - 0002-7537

VL - 32

SP - 1460

JO - Bulletin of the American Astronomical Society

JF - Bulletin of the American Astronomical Society

ER -

Chandra Observations of Arp 220

Abstract

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