<?xml version="1.0" encoding="UTF-8"?>
<!DOCTYPE dataset SYSTEM "http://tarantella.gsfc.nasa.gov/xml/dataset_048.dtd">
<dataset subject="astronomy" xmlns:xlink="http://www.w3.org/XML/XLink/0.9">
	<title>Deep optical imaging of the bright Seyfert galaxy NGC 5548:
a long, very low surface brightness tail.</title>
	<altname type="ADC">J/AJ/116/102</altname>
		<altname type="CDS">J/AJ/116/102</altname>
		<altname type="brief">NGC 5548 BR photometry</altname>
	<reference>
		<source>
<journal>
	<title>Deep optical imaging of the bright Seyfert galaxy NGC 5548:
a long, very low surface brightness tail.</title>
	<author>
			<initial>J</initial>
			<initial>A</initial>
			<lastName>Tyson</lastName></author>
	<author>
			<initial>P</initial>
			<lastName>Fischer</lastName></author>
	<author>
			<initial>P</initial>
			<lastName>Guhathakurta</lastName></author>
	<author>
			<initial>P</initial>
			<lastName>McIlroy</lastName></author>
	<author>
			<initial>R</initial>
			<lastName>Wenk</lastName></author>
	<author>
			<initial>J</initial>
			<lastName>Huchra</lastName></author>
	<author>
			<initial>L</initial>
			<lastName>Macri</lastName></author>
	<author>
			<initial>L</initial>
			<lastName>Neuschaefer</lastName></author>
	<author>
			<initial>V</initial>
			<lastName>Sarajedini</lastName></author>
	<author>
			<initial>K</initial>
			<lastName>Glazebrook</lastName></author>
	<author>
			<initial>K</initial>
			<lastName>Ratnatunga</lastName></author>
	<author>
			<initial>R</initial>
			<lastName>Griffiths</lastName></author>
	<name>Astron. J.</name>
	<volume>116</volume>
	<pageno>102</pageno>
		<date>
			<year>1998</year></date>
	<bibcode>1998AJ....116..102T</bibcode></journal></source>
	<related>
			<holding role="similar">J/A+A/314/43 :  NGC 5548 Profile variability (Kollatschny+ 1996)<xlink:simple href="J/A+A/314/43"/></holding></related></reference>
	<keywords parentListURL="http://messier.gsfc.nasa.gov/xml/keywordlists/adc_keywords.html">
			<keyword xlink:href="Galaxies_Seyfert.html">Galaxies, Seyfert</keyword>
			<keyword xlink:href="Photometry.html">Photometry</keyword></keywords>
	<keywords parentListURL="http://messier.gsfc.nasa.gov/xml/keywordlists/apj_keywords.html">
			<keyword xlink:href="galaxies_clusters_general.html">galaxies: clusters: general</keyword>
			<keyword xlink:href="galaxies_individual_(NGC_5548).html">galaxies: individual (NGC 5548)</keyword>
			<keyword xlink:href="galaxies_Seyfert.html">galaxies: Seyfert</keyword></keywords>
	<descriptions>
				<abstract>
					<para>
    Deep Hubble Space Telescope Wide Field Camera (WFC-1) imaging of a
    region 3.7' east of the V=13mag Seyfert galaxy NGC 5548 in the F555W
    and F785LP bands, and deep ground-based V and I imaging, show a new
    extended, blue, low surface brightness structure, apparently a remnant
    of a tidal interaction associated with NGC 5548. If this straight, low
    surface brightness (V~27-28mag/arcsec^2^) tidal tail is associated
    with NGC 5548, it extends at least 80kpc from it and has an absolute
    magnitude of M_V~-16.4 (H_0_=65km/s/Mpc). Previous imaging surveys of
    Seyfert galaxies would have missed such low surface brightness tails.
    Morphologically similar to some brighter tails seen in other
    interacting systems and in simulations of merging galaxies, this faint
    tail is a useful diagnostic of an earlier interaction and of the
    progenitors' halo-to-disk mass ratios. Luminous ripples and a brighter
    tail wrapped around the galaxy are seen in the inner 1-10kpc region.
    Unresolved blue objects in the long tail have the colors and absolute
    magnitudes of young globular clusters. Taken together, the two tails
    and other features suggest that two spirals merged less than ~1Gyr
    ago. The inner luminosity profile of NGC 5548 is a good fit to a de
    Vaucouleurs profile with r_eff_=5.8kpc. Recent simulations of merged
    galaxies with high-mass halos fail to form lasting tidal tails,
    suggesting that the NGC 5548 progenitor spirals had modest halo
    masses.</para></abstract>
                        <details/></descriptions>
	<tableHead>
		<tableLinks>
				<tableLink xlink:href="table1.dat">
	<title>BR photometry in the NGC 5548 field</title></tableLink></tableLinks>
	<fields>
		<field>
			<name>[TFG98]</name>
			<definition>Star name (NGC 5548-NN)</definition>
			<units>---</units></field>
		<field>
			<name>RAh</name>
			<definition>Right ascension (J2000.0)</definition>
			<units>h</units></field>
		<field>
			<name>RAm</name>
			<definition>Right ascension (J2000.0)</definition>
			<units>min</units></field>
		<field>
			<name>RAs</name>
			<definition>Right ascension (J2000.0)</definition>
			<units>s</units></field>
		<field>
			<name>DE-</name>
			<definition>Declination sign</definition>
			<units>---</units></field>
		<field>
			<name>DEd</name>
			<definition>Declination (J2000.0)</definition>
			<units>deg</units></field>
		<field>
			<name>DEm</name>
			<definition>Declination (J2000.0)</definition>
			<units>arcmin</units></field>
		<field>
			<name>DEs</name>
			<definition>Declination (J2000.0)</definition>
			<units>arcsec</units></field>
		<field>
			<name>Bmag</name>
			<definition>B magnitude</definition>
			<units>mag</units></field>
		<field>
			<name>e_Bmag</name>
			<definition>rms uncertainty on Bmag</definition>
			<units>mag</units></field>
		<field>
			<name>B-R</name>
			<definition>B-R colour index</definition>
			<units>mag</units></field>
		<field>
			<name>e_B-R</name>
			<definition>rms uncertainty on B-R</definition>
			<units>mag</units></field></fields></tableHead>
	
	<history>
		<ingest>
	
			<creator>
				<lastName>James Marcout,  Patricia Bauer</lastName>
				<affiliation>CDS</affiliation></creator>
	<date>
		<year>1998</year><month>Nov</month><day>09</day></date><acknowledgement>From AJ electronic version</acknowledgement></ingest>
		</history>
	<identifier>J_AJ_116_102.xml</identifier></dataset>
