2015ApJ...805..148S


Query : 2015ApJ...805..148S

2015ApJ...805..148S - Astrophys. J., 805, 148 (2015/June-1)

HST images flash ionization of old ejecta by the 2011 eruption of recurrent nova T Pyxidis.

SHARA M.M., ZUREK D., SCHAEFER B.E., BOND H.E., GODON P., LOW M.-M.M., PAGNOTTA A., PRIALNIK D., SION E.M., TORASKAR J. and WILLIAMS R.E.

Abstract (from CDS):

T Pyxidis is the only recurrent nova known to be surrounded by knots of material ejected in previous outbursts. Following the eruption that began on 2011 April 14.29, we obtained seven epochs (from 4 to 383 days after eruption) of Hubble Space Telescope narrowband Hα images of T Pyx. The ionizing flash of radiation from the nova event had no discernible effect on the surrounding ejecta until at least 55 days after the eruption began. Photoionization of hydrogen located north and south of the central star was seen 132 days after the beginning of the eruption. That photoionized hydrogen recombined in the following 51 days, allowing us to determine a hydrogen atom density of at least 7 x 105/cm3 –at least an order of magnitude denser than the previously detected, unresolved [N ii] knots surrounding T Pyx. Material to the northwest and southeast was photoionized, and became bright between 132 and 183 days after the eruption began. Ninety-nine days later that northwest and southeast hydrogen had recombined. Both then (282 days after outburst) and 101 days later, we detected almost no trace of hydrogen emission around T Pyx. We determine that there is a large reservoir of previously unseen, cold diffuse hydrogen overlapping the previously detected, [N ii]-emitting knots of T Pyx ejecta. The mass of this newly detected hydrogen is model-dependent, but is is probably an order of magnitude larger than that of the [N ii] knots. We also determine that there is no significant reservoir of undetected hydrogen-rich ejecta, with density comparable to the flash-ionized ejecta we have detected, from the outer boundaries of the previously detected ejecta out to about twice that distance. The lack of distant ejecta is consistent with the Schaefer et al. scenario for T Pyx, in which the star underwent its first eruption within five years of 1866 after many millennia of quiescence, followed by the six observed recurrent nova eruptions since 1890. The lack of distant ejecta, demonstrated by our observations, is not consistent with scenarios in which T Pyx has been erupting continuously as a recurrent nova for many centuries or millennia.

Abstract Copyright: ∼

Journal keyword(s): ISM: jets and outflows - novae, cataclysmic variables - stars: individual: T Pyxidis - stars: winds, outflows

Simbad objects: 1

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Number of rows : 1
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026
#notes
1 V* T Pyx CV* 09 04 41.5061511720 -32 22 47.502932700           ~ 476 0

Query : 2015ApJ...805..148S

Basic data :
V* T Pyx -- Cataclysmic Binary
Other object types:
otypes_help
V* (AN,V*,...), No* (2024ApJ,NOVA), CV* (2017ARep), * (USNO,Gaia), blu (2019A&A), HS? (2019A&A), NIR (2MASS)
ICRS coord. (ep=J2000) :
09 04 41.5061511720 -32 22 47.502932700 (Optical) [ 0.0157 0.0212 90 ] A 2020yCat.1350....0G
FK4 coord. (ep=B1950 eq=1950) :
09 02 37.1448314262 -32 10 47.531766167 [ 0.0157 0.0212 90 ]
Gal coord. (ep=J2000) :
257.2071797403413 +09.7067371438256 [ 0.0157 0.0212 90 ]
Proper motions mas/yr :
-2.486 0.152 [0.021 0.028 90] A 2020yCat.1350....0G
Parallaxes (mas):
0.3467 [0.0287] A 2020yCat.1350....0G
Fluxes (4) :
G 15.6671 [0.0024] C 2018yCat.1345....0G
J 15.149 [0.049] C 2003yCat.2246....0C
H 14.962 [0.089] C 2003yCat.2246....0C
K 14.684 [0.088] C 2003yCat.2246....0C
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Identifiers (16) :
An access of full data is available using the icon Vizier near the identifier of the catalogue

SV* HV 3348 NOVA Pyx 1944 NOVA Pyx 1920 V* T Pyx
AN 32.1913 NOVA Pyx 1966 NOVA Pyx 2011 AAVSO 0900-31
2MASS J09044150-3222474 NOVA Pyx 1967 TIC 17897279 Gaia DR3 5628258258606112768
NOVA Pyx 1890 NOVA Pyx 1902 USNO-B1.0 0576-00274337 Gaia DR2 5628258258606112768

References (476 between 1850 and 2026) (Total 476)
Simbad bibliographic survey began in 1850 for stars (at least bright stars) and in 1983 for all other objects (outside the solar system).
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Collections of Measurements Description of Measurements

Distance : 2    Plx : 2    PM : 2   

   

Observing logs
Herschel : 7    ISO : 1    IUE : 29   

   


External archives :

Link by name to the catalogue in VizieR :

2MASS J09044150-3222474 USNO-B1.0 0576-00274337 V* T Pyx Gaia DR3 5628258258606112768 Gaia DR2 5628258258606112768

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